{ "cells": [ { "cell_type": "markdown", "metadata": {}, "source": [ "This notebook prepare the catalogues that will be analysed by CIGALE for SED fitting and physical parameter estimation." ] }, { "cell_type": "code", "execution_count": 1, "metadata": { "collapsed": true }, "outputs": [], "source": [ "import numpy as np\n", "import os\n", "os.environ['LOG_LEVEL'] = 'INFO'\n", "import glob\n", "from astropy.table import Table, vstack\n", "\n", "from herschelhelp.filters import correct_galactic_extinction\n", "from herschelhelp.external import convert_table_for_cigale" ] }, { "cell_type": "code", "execution_count": 2, "metadata": { "collapsed": true }, "outputs": [], "source": [ "SUFFIX = '20190207'\n", "file_list = glob.glob('../../dmu32/dmu32_XMM-LSS/data/tiles/xmm-lss_{}_cigale_*.fits'.format(SUFFIX))" ] }, { "cell_type": "code", "execution_count": 3, "metadata": { "collapsed": true }, "outputs": [], "source": [ "#len(master_catalogue)" ] }, { "cell_type": "markdown", "metadata": {}, "source": [ "# Best sources\n", "\n", "Define a good far-IR measurement as:\n", "- an existing flux in the band;\n", "- the flag from XID+ must not be set;\n", "- the signal to noise ratio must be over 2." ] }, { "cell_type": "code", "execution_count": 4, "metadata": { "collapsed": true }, "outputs": [], "source": [ "def main_help_sample(master_catalogue):\n", " good = {}\n", " for band in ['pacs_green', 'pacs_red', 'spire_250', 'spire_350', 'spire_500']:\n", " good[band] = (~np.isnan(master_catalogue['f_{}'.format(band)]) & \n", " ~master_catalogue['flag_{}'.format(band)])\n", " good[band][good[band]] &= (master_catalogue[good[band]]['f_{}'.format(band)] /\n", " master_catalogue[good[band]]['ferr_{}'.format(band)] >= 2)\n", " combined_good = np.sum(list(good.values()), axis=0) >= 2\n", " print(\"Number of good sources: {}\".format(np.sum(combined_good)))\n", " return master_catalogue[combined_good].copy()" ] }, { "cell_type": "markdown", "metadata": {}, "source": [ "We will keep only sources with at leat 2 good far-IR measurements (we may actually use less sources are not all may have a redshift)." ] }, { "cell_type": "code", "execution_count": 5, "metadata": { "collapsed": true }, "outputs": [], "source": [ "# combined_good = np.sum(list(good.values()), axis=0) >= 2" ] }, { "cell_type": "code", "execution_count": 6, "metadata": { "collapsed": true }, "outputs": [], "source": [ "# print(\"Number of good sources: {}\".format(np.sum(combined_good)))" ] }, { "cell_type": "markdown", "metadata": {}, "source": [ "# Main catalogue for CIGALE" ] }, { "cell_type": "code", "execution_count": 7, "metadata": { "collapsed": true }, "outputs": [], "source": [ "# best_catalogue = master_catalogue[combined_good].copy()" ] }, { "cell_type": "code", "execution_count": 8, "metadata": { "collapsed": true }, "outputs": [], "source": [ "# Correction for galactic extinction\n", "#best_catalogue = correct_galactic_extinction(best_catalogue, inplace=True)" ] }, { "cell_type": "code", "execution_count": 9, "metadata": { "collapsed": true, "scrolled": false }, "outputs": [], "source": [ "# Convertion to CIGALE format\n", "#best_catalogue = convert_table_for_cigale(best_catalogue, inplace=True, remove_zerofluxes=True)" ] }, { "cell_type": "markdown", "metadata": {}, "source": [ "## Band selection\n", "\n", "We want to use only one filter for similar bands. We define an order of preference and set to NaN the flux in the lower prefered bands when a prefered band is available. Some band may have a 0 flux, we set there values to NaN." ] }, { "cell_type": "code", "execution_count": 10, "metadata": { "collapsed": true }, "outputs": [], "source": [ "u_bands = [ \"megacam_u\"]\n", "g_bands = [ \"suprime_g\", \"megacam_g\", \"decam_g\", \"gpc1_g\" ]\n", "r_bands = [ \"suprime_r\", \"megacam_r\", \"decam_r\", \"gpc1_r\" ]\n", "i_bands = [ \"suprime_i\", \"megacam_i\", \"decam_i\", \"gpc1_i\" ]\n", "z_bands = [\"vista_z\", \"suprime_z\", \"megacam_z\", \"decam_z\", \"gpc1_z\" ]\n", "y_bands = [\"vista_y\", \"suprime_y\", \"megacam_y\", \"decam_y\", \"gpc1_y\" ]\n", "j_bands = [\"vista_j\", \"wircam_j\", \"ukidss_j\"]\n", "h_bands = [\"vista_h\", \"wircam_h\", \"ukidss_h\"]\n", "k_bands = [\"vista_ks\", \"wircam_ks\"] #, \"ukidss_k\"]\n", "\n", "def remove_unneeded_fluxes(list_of_bands):\n", " for band_idx, band in enumerate(list_of_bands[:-1]):\n", " mask = ~np.isnan(best_catalogue[band])\n", " for lower_band in list_of_bands[band_idx+1:]:\n", " best_catalogue[lower_band][mask] = np.nan\n", " best_catalogue[\"{}_err\".format(lower_band)][mask] = np.nan" ] }, { "cell_type": "code", "execution_count": 11, "metadata": { "collapsed": true }, "outputs": [], "source": [ "# remove_unneeded_fluxes(g_bands)\n", "# remove_unneeded_fluxes(u_bands)\n", "# remove_unneeded_fluxes(r_bands)\n", "# remove_unneeded_fluxes(i_bands)\n", "# remove_unneeded_fluxes(z_bands)\n", "# remove_unneeded_fluxes(y_bands)" ] }, { "cell_type": "code", "execution_count": 12, "metadata": { "collapsed": true }, "outputs": [], "source": [ "#best_catalogue.write(\"data_tmp/CDFS-SWIRE_cigale_best_extcor_20180129.fits\")" ] }, { "cell_type": "code", "execution_count": 13, "metadata": {}, "outputs": [ { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_60.fits:\n", "Number of good sources: 1195\n", "Number of sources with redshift in file 60: 1119\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 9 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 6 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_9.fits:\n", "Number of good sources: 220\n", "Number of sources with redshift in file 9: 217\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 2 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_51.fits:\n", "Number of good sources: 1461\n", "Number of sources with redshift in file 51: 1304\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 48 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 45 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 43 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 43 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 43 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 43 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 39 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 39 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 37 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 37 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 37 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 37 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 37 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 37 sources, the band gpc1_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 37 sources, the band megacam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 37 sources, the band suprime_ip should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 37 sources, the band megacam_y should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 37 sources, the band suprime_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 37 sources, the band decam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 37 sources, the band acs_f814w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_78.fits:\n", "Number of good sources: 324\n", "Number of sources with redshift in file 78: 285\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 2 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_33.fits:\n", "Number of good sources: 635\n", "Number of sources with redshift in file 33: 570\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 3 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band gpc1_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band megacam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_ip should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band megacam_y should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band decam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band acs_f814w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_49.fits:\n", "Number of good sources: 1149\n", "Number of sources with redshift in file 49: 1037\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 30 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 27 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 25 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 25 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 25 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 25 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 20 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 22 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 17 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 17 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 16 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 16 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 15 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 12 sources, the band gpc1_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 12 sources, the band megacam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 12 sources, the band suprime_ip should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 12 sources, the band megacam_y should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 12 sources, the band suprime_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 12 sources, the band decam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 12 sources, the band acs_f814w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_55.fits:\n", "Number of good sources: 1494\n", "Number of sources with redshift in file 55: 1372\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 14 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 9 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 8 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 8 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 8 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 8 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 5 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 5 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 5 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 5 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 5 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 5 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 5 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band gpc1_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band megacam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band suprime_ip should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band megacam_y should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band suprime_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band decam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band acs_f814w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_64.fits:\n", "Number of good sources: 1215\n", "Number of sources with redshift in file 64: 1151\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 14 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 8 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 6 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 6 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 6 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 6 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_37.fits:\n", "Number of good sources: 1100\n", "Number of sources with redshift in file 37: 986\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 6 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 6 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 6 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 6 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 6 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 6 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 5 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 6 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 5 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 5 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 5 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 5 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 5 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 5 sources, the band gpc1_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 5 sources, the band megacam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 5 sources, the band suprime_ip should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 5 sources, the band megacam_y should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 5 sources, the band suprime_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band decam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 5 sources, the band acs_f814w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_70.fits:\n", "Number of good sources: 964\n", "Number of sources with redshift in file 70: 874\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 9 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 8 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 6 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 6 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 6 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 6 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_41.fits:\n", "Number of good sources: 1065\n", "Number of sources with redshift in file 41: 977\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 19 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 13 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 12 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 12 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 11 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 12 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 10 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 10 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 9 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 9 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 9 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 9 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 9 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 6 sources, the band gpc1_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 6 sources, the band megacam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 6 sources, the band suprime_ip should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 6 sources, the band megacam_y should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 6 sources, the band suprime_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 6 sources, the band decam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 6 sources, the band acs_f814w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_23.fits:\n", "Number of good sources: 892\n", "Number of sources with redshift in file 23: 828\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 11 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 7 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 7 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 7 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 7 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 7 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 5 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 5 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band gpc1_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band megacam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band suprime_ip should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band megacam_y should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band suprime_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band decam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band acs_f814w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_68.fits:\n", "Number of good sources: 1024\n", "Number of sources with redshift in file 68: 952\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 7 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 7 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 6 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 6 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 6 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 6 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_81.fits:\n", "Number of good sources: 38\n", "Number of sources with redshift in file 81: 36\n", "Tile xmm-lss_20190207_cigale_1.fits:\n", "Number of good sources: 0\n", "Number of sources with redshift in file 1: 0\n", "Tile xmm-lss_20190207_cigale_59.fits:\n", "Number of good sources: 1376\n", "Number of sources with redshift in file 59: 1268\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 16 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 10 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 6 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 6 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 6 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 6 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 6 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 6 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band gpc1_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band megacam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_ip should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band megacam_y should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band decam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band acs_f814w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_12.fits:\n", "Number of good sources: 422\n", "Number of sources with redshift in file 12: 369\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 1 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_45.fits:\n", "Number of good sources: 1305\n", "Number of sources with redshift in file 45: 1189\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 23 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 20 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 19 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 19 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 18 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 19 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 15 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 15 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 10 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 10 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 10 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 10 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 9 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 8 sources, the band gpc1_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 8 sources, the band megacam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 8 sources, the band suprime_ip should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 8 sources, the band megacam_y should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 8 sources, the band suprime_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 7 sources, the band decam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 8 sources, the band acs_f814w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_74.fits:\n", "Number of good sources: 669\n", "Number of sources with redshift in file 74: 614\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 3 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_5.fits:\n", "Number of good sources: 0\n", "Number of sources with redshift in file 5: 0\n", "Tile xmm-lss_20190207_cigale_16.fits:\n", "Number of good sources: 673\n", "Number of sources with redshift in file 16: 625\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 4 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_27.fits:\n", "Number of good sources: 1014\n", "Number of sources with redshift in file 27: 928\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 8 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 7 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 5 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 5 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 5 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 5 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_85.fits:\n", "Number of good sources: 0\n", "Number of sources with redshift in file 85: 0\n", "Tile xmm-lss_20190207_cigale_71.fits:\n", "Number of good sources: 945\n", "Number of sources with redshift in file 71: 880\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 9 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 9 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 7 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 7 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 7 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 7 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 5 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_40.fits:\n", "Number of good sources: 1119\n", "Number of sources with redshift in file 40: 1018\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 10 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 9 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 6 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 6 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 6 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 6 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band gpc1_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band megacam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band suprime_ip should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band megacam_y should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band suprime_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band decam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band acs_f814w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_69.fits:\n", "Number of good sources: 996\n", "Number of sources with redshift in file 69: 925\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 8 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_22.fits:\n", "Number of good sources: 623\n", "Number of sources with redshift in file 22: 568\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 7 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_80.fits:\n", "Number of good sources: 138\n", "Number of sources with redshift in file 80: 126\n", "Tile xmm-lss_20190207_cigale_0.fits:\n", "Number of good sources: 0\n", "Number of sources with redshift in file 0: 0\n", "Tile xmm-lss_20190207_cigale_13.fits:\n", "Number of good sources: 453\n", "Number of sources with redshift in file 13: 420\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 2 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_58.fits:\n", "Number of good sources: 1442\n", "Number of sources with redshift in file 58: 1305\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 11 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 9 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 6 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 6 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 6 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 6 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 5 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 6 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band gpc1_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band megacam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band suprime_ip should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band megacam_y should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band suprime_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band decam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band acs_f814w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_44.fits:\n", "Number of good sources: 1243\n", "Number of sources with redshift in file 44: 1118\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 13 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 10 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 9 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 9 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 9 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 9 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 6 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 7 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 5 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 5 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 5 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 5 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band gpc1_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band megacam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band suprime_ip should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band megacam_y should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band suprime_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band decam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band acs_f814w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_75.fits:\n", "Number of good sources: 636\n", "Number of sources with redshift in file 75: 585\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 3 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_4.fits:\n", "Number of good sources: 0\n", "Number of sources with redshift in file 4: 0\n", "Tile xmm-lss_20190207_cigale_17.fits:\n", "Number of good sources: 814\n", "Number of sources with redshift in file 17: 743\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 4 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band gpc1_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band megacam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band suprime_ip should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band megacam_y should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band suprime_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band decam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band acs_f814w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_26.fits:\n", "Number of good sources: 1044\n", "Number of sources with redshift in file 26: 964\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 10 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 6 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 5 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 5 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 5 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 5 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band gpc1_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band megacam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_ip should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band megacam_y should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band decam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band acs_f814w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_84.fits:\n", "Number of good sources: 0\n", "Number of sources with redshift in file 84: 0\n", "Tile xmm-lss_20190207_cigale_61.fits:\n", "Number of good sources: 1138\n", "Number of sources with redshift in file 61: 1062\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 11 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 6 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 6 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 6 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 6 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 6 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 5 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_8.fits:\n", "Number of good sources: 104\n", "Number of sources with redshift in file 8: 102\n", "Tile xmm-lss_20190207_cigale_50.fits:\n", "Number of good sources: 1362\n", "Number of sources with redshift in file 50: 1201\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 36 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 33 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 33 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 33 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 33 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 33 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 31 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 31 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 29 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 29 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 29 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 29 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 29 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 27 sources, the band gpc1_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 27 sources, the band megacam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 27 sources, the band suprime_ip should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 27 sources, the band megacam_y should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 27 sources, the band suprime_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 27 sources, the band decam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 27 sources, the band acs_f814w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_32.fits:\n", "Number of good sources: 882\n", "Number of sources with redshift in file 32: 795\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 5 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 5 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 5 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 5 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 5 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 5 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 5 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band gpc1_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band megacam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_ip should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band megacam_y should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band decam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band acs_f814w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_79.fits:\n", "Number of good sources: 258\n", "Number of sources with redshift in file 79: 222\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 1 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_48.fits:\n", "Number of good sources: 1221\n", "Number of sources with redshift in file 48: 1109\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 33 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 30 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 27 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 27 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 27 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 27 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 26 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 26 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 24 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 24 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 24 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 24 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 23 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 17 sources, the band gpc1_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 17 sources, the band megacam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 18 sources, the band suprime_ip should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 17 sources, the band megacam_y should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 17 sources, the band suprime_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 16 sources, the band decam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 16 sources, the band acs_f814w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_54.fits:\n", "Number of good sources: 1410\n", "Number of sources with redshift in file 54: 1287\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 14 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 7 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 5 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 5 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 5 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 5 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band gpc1_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band megacam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band suprime_ip should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band megacam_y should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band suprime_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band decam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band acs_f814w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_65.fits:\n", "Number of good sources: 1178\n", "Number of sources with redshift in file 65: 1098\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 6 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_36.fits:\n", "Number of good sources: 476\n", "Number of sources with redshift in file 36: 429\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 8 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band gpc1_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band megacam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band suprime_ip should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band megacam_y should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band suprime_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band decam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band acs_f814w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_73.fits:\n", "Number of good sources: 778\n", "Number of sources with redshift in file 73: 715\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 10 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 9 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 8 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 9 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 8 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 9 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 6 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 8 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band gpc1_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band megacam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_ip should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band megacam_y should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band decam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band acs_f814w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_38.fits:\n", "Number of good sources: 1106\n", "Number of sources with redshift in file 38: 989\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 10 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 8 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 8 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 8 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 8 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 8 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band gpc1_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band megacam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band suprime_ip should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band megacam_y should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band suprime_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band decam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band acs_f814w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_42.fits:\n", "Number of good sources: 1134\n", "Number of sources with redshift in file 42: 1018\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 9 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 5 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band gpc1_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band megacam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_ip should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band megacam_y should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band decam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band acs_f814w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_82.fits:\n", "Number of good sources: 0\n", "Number of sources with redshift in file 82: 0\n", "Tile xmm-lss_20190207_cigale_20.fits:\n", "Number of good sources: 497\n", "Number of sources with redshift in file 20: 457\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 3 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_11.fits:\n", "Number of good sources: 537\n", "Number of sources with redshift in file 11: 511\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 4 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band gpc1_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band megacam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_ip should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band megacam_y should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band decam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band acs_f814w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_2.fits:\n", "Number of good sources: 0\n", "Number of sources with redshift in file 2: 0\n", "Tile xmm-lss_20190207_cigale_46.fits:\n", "Number of good sources: 1254\n", "Number of sources with redshift in file 46: 1124\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 30 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 24 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 22 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 22 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 21 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 22 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 18 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 18 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 17 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 17 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 17 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 17 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 17 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 14 sources, the band gpc1_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 14 sources, the band megacam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 14 sources, the band suprime_ip should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 14 sources, the band megacam_y should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 14 sources, the band suprime_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 13 sources, the band decam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 13 sources, the band acs_f814w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_77.fits:\n", "Number of good sources: 411\n", "Number of sources with redshift in file 77: 361\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 1 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_15.fits:\n", "Number of good sources: 571\n", "Number of sources with redshift in file 15: 534\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 4 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_6.fits:\n", "Number of good sources: 0\n", "Number of sources with redshift in file 6: 0\n", "Tile xmm-lss_20190207_cigale_86.fits:\n", "Number of good sources: 0\n", "Number of sources with redshift in file 86: 0\n", "Tile xmm-lss_20190207_cigale_24.fits:\n", "Number of good sources: 993\n", "Number of sources with redshift in file 24: 916\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 2 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_28.fits:\n", "Number of good sources: 976\n", "Number of sources with redshift in file 28: 886\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 9 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 6 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 6 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 6 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 6 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 6 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 5 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 5 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band gpc1_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band megacam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_ip should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band megacam_y should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band decam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band acs_f814w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_63.fits:\n", "Number of good sources: 1268\n", "Number of sources with redshift in file 63: 1192\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 11 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 8 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_52.fits:\n", "Number of good sources: 1384\n", "Number of sources with redshift in file 52: 1257\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 8 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band gpc1_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band megacam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band suprime_ip should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band megacam_y should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band suprime_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band decam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band acs_f814w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_19.fits:\n", "Number of good sources: 645\n", "Number of sources with redshift in file 19: 583\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 2 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_30.fits:\n", "Number of good sources: 965\n", "Number of sources with redshift in file 30: 879\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 8 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 8 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 7 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 7 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 7 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 7 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 6 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 7 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 6 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 6 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 5 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 5 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 5 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band gpc1_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band megacam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band suprime_ip should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band megacam_y should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band suprime_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band decam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band acs_f814w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_56.fits:\n", "Number of good sources: 1380\n", "Number of sources with redshift in file 56: 1261\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 11 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 6 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 5 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 5 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 5 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 5 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band gpc1_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band megacam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band suprime_ip should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band megacam_y should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band suprime_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band decam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band acs_f814w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_67.fits:\n", "Number of good sources: 1136\n", "Number of sources with redshift in file 67: 1066\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 9 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_34.fits:\n", "Number of good sources: 787\n", "Number of sources with redshift in file 34: 722\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 5 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band gpc1_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band megacam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_ip should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band megacam_y should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band decam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band acs_f814w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_62.fits:\n", "Number of good sources: 1312\n", "Number of sources with redshift in file 62: 1229\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 15 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 12 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 10 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 10 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 10 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 10 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 6 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 6 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band gpc1_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band megacam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_ip should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band megacam_y should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band decam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band acs_f814w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_29.fits:\n", "Number of good sources: 898\n", "Number of sources with redshift in file 29: 822\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 9 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 7 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 6 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 6 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 6 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 6 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band gpc1_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band megacam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band suprime_ip should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band megacam_y should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band suprime_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band decam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band acs_f814w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_18.fits:\n", "Number of good sources: 930\n", "Number of sources with redshift in file 18: 841\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 6 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 6 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 5 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 5 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 5 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 5 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band gpc1_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band megacam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_ip should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band megacam_y should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band decam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band acs_f814w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_53.fits:\n", "Number of good sources: 1394\n", "Number of sources with redshift in file 53: 1276\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 13 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 12 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 9 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 9 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 8 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 9 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 5 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 5 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band gpc1_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band megacam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band suprime_ip should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band megacam_y should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band suprime_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band decam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band acs_f814w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_31.fits:\n", "Number of good sources: 862\n", "Number of sources with redshift in file 31: 791\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 6 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band gpc1_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band megacam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band suprime_ip should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band megacam_y should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band suprime_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band decam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band acs_f814w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_57.fits:\n", "Number of good sources: 1339\n", "Number of sources with redshift in file 57: 1230\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 12 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 7 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 5 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 5 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 5 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 5 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band gpc1_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band megacam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band suprime_ip should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band megacam_y should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band suprime_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band decam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band acs_f814w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_66.fits:\n", "Number of good sources: 1143\n", "Number of sources with redshift in file 66: 1069\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 7 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 6 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 6 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 6 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 6 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 6 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 5 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 5 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_35.fits:\n", "Number of good sources: 625\n", "Number of sources with redshift in file 35: 566\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 6 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band gpc1_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band megacam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band suprime_ip should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band megacam_y should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band suprime_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band decam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band acs_f814w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_39.fits:\n", "Number of good sources: 1201\n", "Number of sources with redshift in file 39: 1082\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 9 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 8 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 8 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 8 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 7 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 8 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 5 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 5 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_72.fits:\n", "Number of good sources: 917\n", "Number of sources with redshift in file 72: 843\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 11 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 8 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 7 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 7 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 7 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 7 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band megacam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band suprime_ip should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_43.fits:\n", "Number of good sources: 1197\n", "Number of sources with redshift in file 43: 1096\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 23 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 21 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 21 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 21 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 21 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 21 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 13 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 14 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 8 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 8 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 6 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 6 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 6 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band gpc1_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band megacam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band suprime_ip should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band megacam_y should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band suprime_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band decam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band acs_f814w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_83.fits:\n", "Number of good sources: 0\n", "Number of sources with redshift in file 83: 0\n", "Tile xmm-lss_20190207_cigale_21.fits:\n", "Number of good sources: 723\n", "Number of sources with redshift in file 21: 670\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 3 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band gpc1_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band megacam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band suprime_ip should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band megacam_y should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band suprime_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band decam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band acs_f814w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_10.fits:\n", "Number of good sources: 390\n", "Number of sources with redshift in file 10: 386\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 2 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_3.fits:\n", "Number of good sources: 0\n", "Number of sources with redshift in file 3: 0\n", "Tile xmm-lss_20190207_cigale_47.fits:\n", "Number of good sources: 1270\n", "Number of sources with redshift in file 47: 1141\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 27 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 23 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 21 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 21 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 21 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 21 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 17 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 18 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 16 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 16 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 16 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 16 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 15 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 5 sources, the band gpc1_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 5 sources, the band megacam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 5 sources, the band suprime_ip should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 5 sources, the band megacam_y should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 5 sources, the band suprime_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band decam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band acs_f814w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_76.fits:\n", "Number of good sources: 589\n", "Number of sources with redshift in file 76: 534\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 3 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_14.fits:\n", "Number of good sources: 505\n", "Number of sources with redshift in file 14: 468\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 5 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_7.fits:\n", "Number of good sources: 13\n", "Number of sources with redshift in file 7: 13\n", "Tile xmm-lss_20190207_cigale_87.fits:\n", "Number of good sources: 0\n", "Number of sources with redshift in file 87: 0\n", "Tile xmm-lss_20190207_cigale_25.fits:\n", "Number of good sources: 1055\n", "Number of sources with redshift in file 25: 959\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 12 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 9 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 8 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 8 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 8 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 8 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 7 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 7 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 6 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 6 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 6 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 6 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 5 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band gpc1_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band megacam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band suprime_ip should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band megacam_y should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band suprime_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band decam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band acs_f814w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] } ], "source": [ "cigale_input = Table()\n", "\n", "for tile in file_list:\n", " \n", " file_num = tile.split('_')[4].split('.')[0]\n", " print(\"Tile {}:\".format(tile.split('/')[-1]))\n", " best_catalogue = Table.read(tile)\n", " best_catalogue = main_help_sample(best_catalogue)\n", "\n", "\n", " best_catalogue = best_catalogue[~np.isnan(best_catalogue[\"redshift\"])]\n", "\n", " print(\"Number of sources with redshift in file {}: {}\".format(file_num, len(best_catalogue)))\n", "\n", " # Correction for galactic extinction\n", " best_catalogue = correct_galactic_extinction(best_catalogue, inplace=True)\n", "\n", " # Convertion to CIGALE format\n", "\n", " best_catalogue = convert_table_for_cigale(best_catalogue, inplace=True, remove_zerofluxes=True)\n", "\n", " remove_unneeded_fluxes(g_bands)\n", " remove_unneeded_fluxes(u_bands)\n", " remove_unneeded_fluxes(r_bands)\n", " remove_unneeded_fluxes(i_bands)\n", " remove_unneeded_fluxes(z_bands)\n", " remove_unneeded_fluxes(y_bands)\n", " remove_unneeded_fluxes(j_bands)\n", " remove_unneeded_fluxes(h_bands)\n", " remove_unneeded_fluxes(k_bands)\n", "\n", " cigale_input = vstack([cigale_input, best_catalogue])\n", " #best_catalogue.write(\"data_tmp/tiles/XMM-LSS_cigale_best_extcor_{}_{}.fits\".format(SUFFIX, file_num), overwrite=True)\n", " \n", " \n", "cigale_input.write(\"data_tmp/xmm-lss_cigale_best_extcor_{}.fits\".format(SUFFIX), overwrite=True)" ] }, { "cell_type": "markdown", "metadata": {}, "source": [ "# All optnir objects with photo-z" ] }, { "cell_type": "code", "execution_count": 14, "metadata": {}, "outputs": [ { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_60.fits:\n", "Number of sources with redshift in file 60: 22796\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 566 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 437 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 344 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 346 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 341 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 345 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 151 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 193 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 42 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 33 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 28 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 19 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 10 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band gpc1_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band megacam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_ip should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band megacam_y should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band decam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band acs_f814w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_9.fits:\n", "Number of sources with redshift in file 9: 3690\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 21 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 20 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 19 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 19 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 19 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 19 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 18 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 19 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 18 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 18 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 18 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 18 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 18 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 15 sources, the band gpc1_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 15 sources, the band megacam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 15 sources, the band suprime_ip should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 15 sources, the band megacam_y should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 15 sources, the band suprime_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 15 sources, the band decam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 15 sources, the band acs_f814w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_51.fits:\n", "Number of sources with redshift in file 51: 20534\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 368 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 335 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 318 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 318 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 318 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 318 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 286 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 289 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 277 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 273 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 273 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 273 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 271 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 257 sources, the band gpc1_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 257 sources, the band megacam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 257 sources, the band suprime_ip should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 257 sources, the band megacam_y should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 257 sources, the band suprime_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 249 sources, the band decam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 253 sources, the band acs_f814w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_78.fits:\n", "Number of sources with redshift in file 78: 23861\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 460 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 366 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 296 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 298 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 293 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 296 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 130 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 156 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 16 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 11 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 10 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 9 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_33.fits:\n", "Number of sources with redshift in file 33: 14214\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 173 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 160 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 155 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 155 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 153 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 155 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 131 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 136 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 106 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 105 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 101 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 97 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 77 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 11 sources, the band gpc1_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 15 sources, the band megacam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 16 sources, the band suprime_ip should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 13 sources, the band megacam_y should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 10 sources, the band suprime_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 6 sources, the band decam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 7 sources, the band acs_f814w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_49.fits:\n", "Number of sources with redshift in file 49: 17161\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 311 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 262 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 236 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 236 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 236 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 236 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 202 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 208 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 183 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 182 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 180 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 178 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 160 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 128 sources, the band gpc1_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 128 sources, the band megacam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 129 sources, the band suprime_ip should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 128 sources, the band megacam_y should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 128 sources, the band suprime_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 118 sources, the band decam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 125 sources, the band acs_f814w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_55.fits:\n", "Number of sources with redshift in file 55: 22176\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 79 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 50 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 31 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 32 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 31 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 32 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 14 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 15 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 14 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 14 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 13 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 13 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 13 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 12 sources, the band gpc1_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 12 sources, the band megacam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 12 sources, the band suprime_ip should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 12 sources, the band megacam_y should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 12 sources, the band suprime_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 11 sources, the band decam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 11 sources, the band acs_f814w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_64.fits:\n", "Number of sources with redshift in file 64: 22568\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 609 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 514 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 443 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 445 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 437 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 445 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 230 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 280 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 92 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 78 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 68 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 49 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 24 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band gpc1_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band megacam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band suprime_ip should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band megacam_y should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band decam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band acs_f814w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_37.fits:\n", "Number of sources with redshift in file 37: 22229\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 224 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 191 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 159 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 162 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 159 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 160 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 108 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 115 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 68 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 64 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 60 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 55 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 44 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 22 sources, the band gpc1_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 22 sources, the band megacam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 22 sources, the band suprime_ip should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 22 sources, the band megacam_y should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 22 sources, the band suprime_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 16 sources, the band decam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 19 sources, the band acs_f814w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_70.fits:\n", "Number of sources with redshift in file 70: 22532\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 615 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 499 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 436 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 437 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 431 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 436 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 206 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 252 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 59 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 50 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 41 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 29 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 5 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_41.fits:\n", "Number of sources with redshift in file 41: 19581\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 452 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 412 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 373 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 375 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 372 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 373 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 313 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 328 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 253 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 247 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 240 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 230 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 191 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 39 sources, the band gpc1_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 41 sources, the band megacam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 41 sources, the band suprime_ip should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 41 sources, the band megacam_y should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 39 sources, the band suprime_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 34 sources, the band decam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 35 sources, the band acs_f814w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_23.fits:\n", "Number of sources with redshift in file 23: 21659\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 225 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 206 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 186 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 187 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 186 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 187 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 151 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 159 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 117 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 115 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 113 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 107 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 84 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 18 sources, the band gpc1_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 20 sources, the band megacam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 20 sources, the band suprime_ip should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 18 sources, the band megacam_y should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 18 sources, the band suprime_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 13 sources, the band decam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 16 sources, the band acs_f814w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_68.fits:\n", "Number of sources with redshift in file 68: 23461\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 562 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 470 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 397 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 405 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 393 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 399 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 200 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 241 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 67 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 53 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 49 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 34 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 12 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band gpc1_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band megacam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_ip should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band megacam_y should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_81.fits:\n", "Number of sources with redshift in file 81: 6426\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 23 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 11 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 7 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 7 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 7 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 7 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_1.fits:\n", "Number of sources with redshift in file 1: 2320\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 2 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_59.fits:\n", "Number of sources with redshift in file 59: 24508\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 107 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 63 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 25 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 26 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 23 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 25 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 13 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 13 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 7 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 7 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 7 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 6 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 6 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band gpc1_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band megacam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band suprime_ip should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band megacam_y should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band suprime_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band decam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band acs_f814w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_12.fits:\n", "Number of sources with redshift in file 12: 5102\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 115 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 103 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 100 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 100 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 100 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 100 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 84 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 86 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 67 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 65 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 63 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 56 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 43 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 16 sources, the band gpc1_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 16 sources, the band megacam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 16 sources, the band suprime_ip should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 16 sources, the band megacam_y should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 16 sources, the band suprime_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 14 sources, the band decam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 14 sources, the band acs_f814w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_45.fits:\n", "Number of sources with redshift in file 45: 18378\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 360 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 295 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 245 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 247 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 241 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 245 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 148 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 160 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 89 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 88 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 86 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 84 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 78 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 62 sources, the band gpc1_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 62 sources, the band megacam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 62 sources, the band suprime_ip should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 62 sources, the band megacam_y should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 62 sources, the band suprime_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 58 sources, the band decam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 59 sources, the band acs_f814w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_74.fits:\n", "Number of sources with redshift in file 74: 23986\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 555 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 456 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 392 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 392 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 390 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 392 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 187 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 232 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 57 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 51 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 45 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 36 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 10 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_5.fits:\n", "Number of sources with redshift in file 5: 3791\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 1 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_16.fits:\n", "Number of sources with redshift in file 16: 22439\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 393 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 355 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 323 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 324 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 320 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 324 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 263 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 272 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 207 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 196 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 187 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 174 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 128 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 71 sources, the band gpc1_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 73 sources, the band megacam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 73 sources, the band suprime_ip should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 71 sources, the band megacam_y should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 70 sources, the band suprime_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 63 sources, the band decam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 66 sources, the band acs_f814w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_27.fits:\n", "Number of sources with redshift in file 27: 22265\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 206 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 179 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 163 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 163 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 163 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 163 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 123 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 133 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 100 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 98 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 94 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 88 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 68 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 12 sources, the band gpc1_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 12 sources, the band megacam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 12 sources, the band suprime_ip should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 12 sources, the band megacam_y should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 12 sources, the band suprime_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 5 sources, the band decam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 10 sources, the band acs_f814w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_85.fits:\n", "Number of sources with redshift in file 85: 3522\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 13 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 8 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 5 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_71.fits:\n", "Number of sources with redshift in file 71: 23740\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 560 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 456 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 386 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 389 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 385 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 389 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 190 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 238 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 48 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 41 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 34 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 27 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 11 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_40.fits:\n", "Number of sources with redshift in file 40: 18913\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 394 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 342 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 314 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 315 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 310 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 314 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 253 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 261 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 201 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 196 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 189 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 184 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 144 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 16 sources, the band gpc1_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 19 sources, the band megacam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 19 sources, the band suprime_ip should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 17 sources, the band megacam_y should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 15 sources, the band suprime_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 11 sources, the band decam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 14 sources, the band acs_f814w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_69.fits:\n", "Number of sources with redshift in file 69: 22689\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 582 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 502 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 424 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 426 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 423 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 425 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 202 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 261 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 58 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 51 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 40 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 29 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 8 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band gpc1_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band megacam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_ip should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band megacam_y should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band decam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band acs_f814w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_22.fits:\n", "Number of sources with redshift in file 22: 15987\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 158 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 138 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 128 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 128 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 127 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 128 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 106 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 111 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 85 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 83 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 80 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 74 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 62 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 22 sources, the band gpc1_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 23 sources, the band megacam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 25 sources, the band suprime_ip should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 23 sources, the band megacam_y should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 22 sources, the band suprime_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 15 sources, the band decam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 18 sources, the band acs_f814w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_80.fits:\n", "Number of sources with redshift in file 80: 23601\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 74 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 44 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 20 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 20 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 17 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 20 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_0.fits:\n", "Number of sources with redshift in file 0: 3673\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 4 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_13.fits:\n", "Number of sources with redshift in file 13: 15669\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 253 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 229 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 219 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 219 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 219 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 219 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 185 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 191 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 148 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 141 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 141 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 132 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 102 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 24 sources, the band gpc1_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 26 sources, the band megacam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 26 sources, the band suprime_ip should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 24 sources, the band megacam_y should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 24 sources, the band suprime_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 21 sources, the band decam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 22 sources, the band acs_f814w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_58.fits:\n", "Number of sources with redshift in file 58: 22543\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 87 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 60 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 38 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 40 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 38 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 39 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 20 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 22 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 16 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 16 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 16 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 15 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 15 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 10 sources, the band gpc1_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 10 sources, the band megacam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 10 sources, the band suprime_ip should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 10 sources, the band megacam_y should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 10 sources, the band suprime_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 5 sources, the band decam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 10 sources, the band acs_f814w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_44.fits:\n", "Number of sources with redshift in file 44: 17803\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 307 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 262 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 212 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 213 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 205 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 213 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 126 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 142 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 85 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 81 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 74 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 71 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 63 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 13 sources, the band gpc1_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 13 sources, the band megacam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 13 sources, the band suprime_ip should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 13 sources, the band megacam_y should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 13 sources, the band suprime_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 9 sources, the band decam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 11 sources, the band acs_f814w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_75.fits:\n", "Number of sources with redshift in file 75: 25017\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 631 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 518 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 439 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 446 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 434 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 442 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 205 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 251 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 55 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 41 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 37 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 29 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 12 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band gpc1_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band megacam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_ip should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band megacam_y should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band decam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band acs_f814w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_4.fits:\n", "Number of sources with redshift in file 4: 3427\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 3 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_17.fits:\n", "Number of sources with redshift in file 17: 24425\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 259 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 220 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 178 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 181 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 174 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 179 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 131 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 142 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 92 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 89 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 86 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 81 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 64 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 28 sources, the band gpc1_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 29 sources, the band megacam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 29 sources, the band suprime_ip should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 29 sources, the band megacam_y should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 28 sources, the band suprime_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 26 sources, the band decam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 28 sources, the band acs_f814w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_26.fits:\n", "Number of sources with redshift in file 26: 21847\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 174 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 153 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 143 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 143 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 143 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 143 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 111 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 117 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 85 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 85 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 79 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 76 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 62 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 11 sources, the band gpc1_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 15 sources, the band megacam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 15 sources, the band suprime_ip should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 14 sources, the band megacam_y should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 11 sources, the band suprime_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 6 sources, the band decam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 8 sources, the band acs_f814w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_84.fits:\n", "Number of sources with redshift in file 84: 2536\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 5 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band gpc1_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band megacam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_ip should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band megacam_y should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band decam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band acs_f814w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_61.fits:\n", "Number of sources with redshift in file 61: 23217\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 675 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 572 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 485 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 488 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 478 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 486 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 220 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 280 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 53 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 43 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 39 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 26 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 11 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band megacam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_ip should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_8.fits:\n", "Number of sources with redshift in file 8: 3638\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 1 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_50.fits:\n", "Number of sources with redshift in file 50: 19124\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 357 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 328 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 313 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 313 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 313 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 313 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 298 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 299 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 289 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 289 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 289 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 288 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 281 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 240 sources, the band gpc1_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 240 sources, the band megacam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 240 sources, the band suprime_ip should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 240 sources, the band megacam_y should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 240 sources, the band suprime_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 238 sources, the band decam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 239 sources, the band acs_f814w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_32.fits:\n", "Number of sources with redshift in file 32: 18779\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 222 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 206 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 197 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 198 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 196 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 198 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 165 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 169 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 136 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 131 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 125 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 117 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 90 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 30 sources, the band gpc1_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 31 sources, the band megacam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 32 sources, the band suprime_ip should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 31 sources, the band megacam_y should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 29 sources, the band suprime_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 15 sources, the band decam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 21 sources, the band acs_f814w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_79.fits:\n", "Number of sources with redshift in file 79: 26159\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 96 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 60 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 34 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 35 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 32 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 35 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 11 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 15 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 9 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 9 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 9 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 9 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 9 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_48.fits:\n", "Number of sources with redshift in file 48: 17393\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 344 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 287 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 247 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 248 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 245 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 247 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 197 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 204 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 184 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 184 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 183 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 177 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 158 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 98 sources, the band gpc1_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 98 sources, the band megacam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 99 sources, the band suprime_ip should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 98 sources, the band megacam_y should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 98 sources, the band suprime_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 89 sources, the band decam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 95 sources, the band acs_f814w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_54.fits:\n", "Number of sources with redshift in file 54: 21615\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 72 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 42 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 27 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 28 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 26 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 28 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 16 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 16 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 10 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 9 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 9 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 9 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 9 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 8 sources, the band gpc1_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 8 sources, the band megacam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 8 sources, the band suprime_ip should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 8 sources, the band megacam_y should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 8 sources, the band suprime_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 7 sources, the band decam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 8 sources, the band acs_f814w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_65.fits:\n", "Number of sources with redshift in file 65: 23408\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 592 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 524 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 463 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 468 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 460 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 467 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 282 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 326 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 98 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 85 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 72 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 59 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 24 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band gpc1_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band megacam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_ip should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band megacam_y should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band acs_f814w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_36.fits:\n", "Number of sources with redshift in file 36: 9948\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 131 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 114 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 96 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 98 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 94 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 96 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 71 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 78 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 54 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 52 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 49 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 48 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 36 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 10 sources, the band gpc1_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 13 sources, the band megacam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 13 sources, the band suprime_ip should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 12 sources, the band megacam_y should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 10 sources, the band suprime_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 8 sources, the band decam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 9 sources, the band acs_f814w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_73.fits:\n", "Number of sources with redshift in file 73: 24272\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 591 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 491 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 425 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 431 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 421 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 428 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 202 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 262 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 71 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 63 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 49 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 41 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 15 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band gpc1_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band megacam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_ip should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band megacam_y should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band decam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band acs_f814w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_38.fits:\n", "Number of sources with redshift in file 38: 22025\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 217 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 173 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 147 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 149 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 147 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 148 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 95 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 98 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 54 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 53 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 48 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 43 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 33 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 7 sources, the band gpc1_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 8 sources, the band megacam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 8 sources, the band suprime_ip should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 7 sources, the band megacam_y should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 7 sources, the band suprime_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 6 sources, the band decam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 6 sources, the band acs_f814w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_42.fits:\n", "Number of sources with redshift in file 42: 17206\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 378 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 343 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 321 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 322 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 321 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 322 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 276 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 289 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 212 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 209 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 207 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 196 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 152 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 23 sources, the band gpc1_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 23 sources, the band megacam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 23 sources, the band suprime_ip should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 23 sources, the band megacam_y should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 23 sources, the band suprime_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 18 sources, the band decam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 21 sources, the band acs_f814w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_82.fits:\n", "Number of sources with redshift in file 82: 1983\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 4 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_20.fits:\n", "Number of sources with redshift in file 20: 11841\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 142 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 124 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 106 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 107 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 105 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 107 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 82 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 88 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 60 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 59 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 56 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 53 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 39 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 10 sources, the band gpc1_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 10 sources, the band megacam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 10 sources, the band suprime_ip should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 10 sources, the band megacam_y should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 10 sources, the band suprime_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 9 sources, the band decam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 10 sources, the band acs_f814w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_11.fits:\n", "Number of sources with redshift in file 11: 4322\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 43 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 37 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 36 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 36 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 36 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 36 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 36 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 36 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 34 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 34 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 32 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 32 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 26 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 12 sources, the band gpc1_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 12 sources, the band megacam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 12 sources, the band suprime_ip should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 12 sources, the band megacam_y should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 12 sources, the band suprime_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 12 sources, the band decam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 12 sources, the band acs_f814w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_2.fits:\n", "Number of sources with redshift in file 2: 4288\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 8 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_46.fits:\n", "Number of sources with redshift in file 46: 18523\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 304 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 244 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 199 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 202 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 196 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 202 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 140 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 147 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 105 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 101 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 101 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 100 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 98 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 73 sources, the band gpc1_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 75 sources, the band megacam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 75 sources, the band suprime_ip should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 74 sources, the band megacam_y should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 72 sources, the band suprime_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 66 sources, the band decam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 69 sources, the band acs_f814w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_77.fits:\n", "Number of sources with redshift in file 77: 23592\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 644 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 523 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 440 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 445 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 434 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 444 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 183 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 233 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 29 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 23 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 17 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 13 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 9 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band gpc1_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band megacam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band suprime_ip should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band megacam_y should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band decam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band acs_f814w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_15.fits:\n", "Number of sources with redshift in file 15: 20584\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 322 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 293 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 257 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 260 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 254 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 258 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 218 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 223 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 186 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 181 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 178 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 170 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 145 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 75 sources, the band gpc1_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 76 sources, the band megacam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 76 sources, the band suprime_ip should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 75 sources, the band megacam_y should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 74 sources, the band suprime_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 71 sources, the band decam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 73 sources, the band acs_f814w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_6.fits:\n", "Number of sources with redshift in file 6: 2983\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 3 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_86.fits:\n", "Number of sources with redshift in file 86: 1742\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 8 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 5 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 5 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 5 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 5 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 5 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 5 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 5 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 5 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band gpc1_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band megacam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band suprime_ip should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band megacam_y should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band acs_f814w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_24.fits:\n", "Number of sources with redshift in file 24: 22513\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 200 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 184 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 177 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 177 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 175 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 177 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 135 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 147 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 108 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 106 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 104 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 91 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 72 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 12 sources, the band gpc1_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 18 sources, the band megacam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 18 sources, the band suprime_ip should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 13 sources, the band megacam_y should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 12 sources, the band suprime_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 10 sources, the band decam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 11 sources, the band acs_f814w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_28.fits:\n", "Number of sources with redshift in file 28: 21914\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 229 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 194 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 172 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 172 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 170 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 172 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 139 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 148 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 109 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 102 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 99 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 93 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 67 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 15 sources, the band gpc1_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 15 sources, the band megacam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 15 sources, the band suprime_ip should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 15 sources, the band megacam_y should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 15 sources, the band suprime_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 8 sources, the band decam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 14 sources, the band acs_f814w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_63.fits:\n", "Number of sources with redshift in file 63: 22948\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 620 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 514 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 436 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 440 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 434 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 440 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 246 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 293 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 87 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 73 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 65 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 53 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 13 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_52.fits:\n", "Number of sources with redshift in file 52: 20663\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 80 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 47 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 23 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 24 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 23 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 24 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 12 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 13 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 11 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 11 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 11 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 11 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 11 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 9 sources, the band gpc1_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 9 sources, the band megacam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 9 sources, the band suprime_ip should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 9 sources, the band megacam_y should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 8 sources, the band suprime_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 7 sources, the band decam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 8 sources, the band acs_f814w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_19.fits:\n", "Number of sources with redshift in file 19: 16112\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 175 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 133 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 108 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 108 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 107 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 108 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 70 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 74 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 44 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 43 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 40 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 37 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 27 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 5 sources, the band gpc1_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 5 sources, the band megacam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 5 sources, the band suprime_ip should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 5 sources, the band megacam_y should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band suprime_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band decam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band acs_f814w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_30.fits:\n", "Number of sources with redshift in file 30: 20282\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 240 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 204 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 190 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 193 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 189 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 192 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 152 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 166 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 128 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 127 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 121 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 111 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 97 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 27 sources, the band gpc1_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 27 sources, the band megacam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 28 sources, the band suprime_ip should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 27 sources, the band megacam_y should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 25 sources, the band suprime_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 19 sources, the band decam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 20 sources, the band acs_f814w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_56.fits:\n", "Number of sources with redshift in file 56: 21004\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 95 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 67 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 39 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 41 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 39 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 40 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 28 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 29 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 23 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 23 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 23 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 22 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 21 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 18 sources, the band gpc1_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 18 sources, the band megacam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 18 sources, the band suprime_ip should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 18 sources, the band megacam_y should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 18 sources, the band suprime_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 11 sources, the band decam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 17 sources, the band acs_f814w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_67.fits:\n", "Number of sources with redshift in file 67: 23856\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 573 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 482 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 415 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 418 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 414 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 416 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 231 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 275 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 68 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 60 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 52 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 42 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 19 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band gpc1_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band megacam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band suprime_ip should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band megacam_y should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band suprime_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band decam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band acs_f814w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_34.fits:\n", "Number of sources with redshift in file 34: 16209\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 164 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 149 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 136 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 137 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 136 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 137 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 111 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 119 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 93 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 89 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 86 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 82 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 71 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 15 sources, the band gpc1_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 19 sources, the band megacam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 19 sources, the band suprime_ip should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 16 sources, the band megacam_y should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 15 sources, the band suprime_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 9 sources, the band decam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 13 sources, the band acs_f814w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_62.fits:\n", "Number of sources with redshift in file 62: 24139\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 614 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 511 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 436 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 441 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 431 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 440 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 221 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 258 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 69 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 62 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 55 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 42 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 18 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band gpc1_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band megacam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band suprime_ip should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band megacam_y should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band suprime_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band decam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band acs_f814w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_29.fits:\n", "Number of sources with redshift in file 29: 21238\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 258 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 221 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 206 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 208 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 203 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 206 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 164 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 171 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 129 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 126 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 121 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 116 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 99 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 16 sources, the band gpc1_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 18 sources, the band megacam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 19 sources, the band suprime_ip should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 17 sources, the band megacam_y should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 15 sources, the band suprime_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 10 sources, the band decam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 11 sources, the band acs_f814w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_18.fits:\n", "Number of sources with redshift in file 18: 24117\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 220 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 176 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 152 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 153 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 150 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 152 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 94 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 98 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 50 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 48 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 47 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 44 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 37 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 20 sources, the band gpc1_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 20 sources, the band megacam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 20 sources, the band suprime_ip should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 20 sources, the band megacam_y should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 20 sources, the band suprime_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 18 sources, the band decam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 19 sources, the band acs_f814w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_53.fits:\n", "Number of sources with redshift in file 53: 20622\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 76 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 48 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 31 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 32 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 29 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 32 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 14 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 14 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 14 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 14 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 13 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 13 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 12 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 11 sources, the band gpc1_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 12 sources, the band megacam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 12 sources, the band suprime_ip should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 12 sources, the band megacam_y should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 11 sources, the band suprime_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 9 sources, the band decam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 10 sources, the band acs_f814w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_31.fits:\n", "Number of sources with redshift in file 31: 19437\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 255 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 234 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 215 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 216 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 213 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 216 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 165 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 182 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 123 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 118 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 112 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 103 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 78 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 15 sources, the band gpc1_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 16 sources, the band megacam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 16 sources, the band suprime_ip should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 16 sources, the band megacam_y should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 15 sources, the band suprime_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 13 sources, the band decam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 13 sources, the band acs_f814w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_57.fits:\n", "Number of sources with redshift in file 57: 21130\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 92 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 61 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 38 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 41 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 37 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 40 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 23 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 24 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 20 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 20 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 19 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 19 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 19 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 16 sources, the band gpc1_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 17 sources, the band megacam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 17 sources, the band suprime_ip should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 17 sources, the band megacam_y should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 16 sources, the band suprime_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 13 sources, the band decam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 15 sources, the band acs_f814w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_66.fits:\n", "Number of sources with redshift in file 66: 23957\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 569 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 493 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 409 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 416 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 406 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 411 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 233 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 277 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 85 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 67 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 56 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 45 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 18 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_35.fits:\n", "Number of sources with redshift in file 35: 13317\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 136 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 123 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 113 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 114 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 113 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 114 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 97 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 102 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 84 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 79 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 78 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 74 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 64 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 23 sources, the band gpc1_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 23 sources, the band megacam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 23 sources, the band suprime_ip should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 23 sources, the band megacam_y should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 23 sources, the band suprime_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 20 sources, the band decam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 22 sources, the band acs_f814w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_39.fits:\n", "Number of sources with redshift in file 39: 19537\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 354 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 309 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 280 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 282 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 279 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 281 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 209 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 227 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 156 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 156 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 152 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 143 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 119 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 21 sources, the band gpc1_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 21 sources, the band megacam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 21 sources, the band suprime_ip should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 21 sources, the band megacam_y should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 20 sources, the band suprime_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 9 sources, the band decam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 12 sources, the band acs_f814w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_72.fits:\n", "Number of sources with redshift in file 72: 24289\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 612 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 532 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 448 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 453 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 446 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 452 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 231 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 285 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 74 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 59 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 45 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 36 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 19 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band gpc1_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band megacam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band suprime_ip should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band megacam_y should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_43.fits:\n", "Number of sources with redshift in file 43: 16545\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 393 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 355 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 327 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 329 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 327 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 329 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 287 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 304 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 220 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 212 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 206 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 197 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 149 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 31 sources, the band gpc1_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 31 sources, the band megacam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 31 sources, the band suprime_ip should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 31 sources, the band megacam_y should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 29 sources, the band suprime_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 25 sources, the band decam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 27 sources, the band acs_f814w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_83.fits:\n", "Number of sources with redshift in file 83: 2224\n", "Tile xmm-lss_20190207_cigale_21.fits:\n", "Number of sources with redshift in file 21: 17945\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 146 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 128 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 117 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 119 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 117 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 117 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 90 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 99 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 69 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 63 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 59 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 57 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 49 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 18 sources, the band gpc1_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 21 sources, the band megacam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 22 sources, the band suprime_ip should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 19 sources, the band megacam_y should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 18 sources, the band suprime_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 13 sources, the band decam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 16 sources, the band acs_f814w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_10.fits:\n", "Number of sources with redshift in file 10: 3616\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 26 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 21 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 20 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 20 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 20 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 20 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 20 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 20 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 20 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 20 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 20 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 20 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 13 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 9 sources, the band gpc1_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 9 sources, the band megacam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 9 sources, the band suprime_ip should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 9 sources, the band megacam_y should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 9 sources, the band suprime_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 9 sources, the band decam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 9 sources, the band acs_f814w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_3.fits:\n", "Number of sources with redshift in file 3: 3223\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 5 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_47.fits:\n", "Number of sources with redshift in file 47: 18709\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 348 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 295 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 257 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 258 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 256 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 258 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 201 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 211 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 178 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 178 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 177 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 173 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 157 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 55 sources, the band gpc1_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 56 sources, the band megacam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 57 sources, the band suprime_ip should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 56 sources, the band megacam_y should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 54 sources, the band suprime_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 41 sources, the band decam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 50 sources, the band acs_f814w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_76.fits:\n", "Number of sources with redshift in file 76: 25649\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 701 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 581 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 501 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 502 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 495 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 501 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 243 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 303 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 58 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 50 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 42 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 32 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 14 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band gpc1_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band megacam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band suprime_ip should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band megacam_y should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band suprime_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band decam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band acs_f814w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_14.fits:\n", "Number of sources with redshift in file 14: 17550\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 195 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 177 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 165 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 165 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 165 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 165 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 137 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 140 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 109 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 107 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 105 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 102 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 80 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 9 sources, the band gpc1_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 10 sources, the band megacam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 10 sources, the band suprime_ip should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 10 sources, the band megacam_y should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 9 sources, the band suprime_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 7 sources, the band decam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 8 sources, the band acs_f814w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_7.fits:\n", "Number of sources with redshift in file 7: 2890\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 3 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_87.fits:\n", "Number of sources with redshift in file 87: 217\n", "Tile xmm-lss_20190207_cigale_25.fits:\n", "Number of sources with redshift in file 25: 23286\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 183 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 161 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 148 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 148 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 148 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 148 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 129 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 130 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 98 sources, the band suprime_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 95 sources, the band gpc1_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 94 sources, the band megacam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 92 sources, the band decam_r should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 74 sources, the band suprime_rc should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 17 sources, the band gpc1_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 17 sources, the band megacam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 17 sources, the band suprime_ip should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 17 sources, the band megacam_y should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 15 sources, the band suprime_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 8 sources, the band decam_i should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 13 sources, the band acs_f814w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] } ], "source": [ "cigale_input = Table()\n", "\n", "for tile in file_list:\n", " \n", " file_num = tile.split('_')[4].split('.')[0]\n", " print(\"Tile {}:\".format(tile.split('/')[-1]))\n", " best_catalogue = Table.read(tile)\n", " \n", " #best_catalogue = main_help_sample(best_catalogue)\n", " optnir = ((best_catalogue['flag_optnir_det'] == 3) \n", " | (best_catalogue['flag_optnir_det'] == 7))\n", " \n", " best_catalogue = best_catalogue[optnir]\n", "\n", " best_catalogue = best_catalogue[~np.isnan(best_catalogue[\"redshift\"])]\n", "\n", " print(\"Number of sources with redshift in file {}: {}\".format(file_num, len(best_catalogue)))\n", "\n", " # Correction for galactic extinction\n", " best_catalogue = correct_galactic_extinction(best_catalogue, inplace=True)\n", "\n", " # Convertion to CIGALE format\n", "\n", " best_catalogue = convert_table_for_cigale(best_catalogue, inplace=True, remove_zerofluxes=True)\n", "\n", " remove_unneeded_fluxes(g_bands)\n", " remove_unneeded_fluxes(u_bands)\n", " remove_unneeded_fluxes(r_bands)\n", " remove_unneeded_fluxes(i_bands)\n", " remove_unneeded_fluxes(z_bands)\n", " remove_unneeded_fluxes(y_bands)\n", " remove_unneeded_fluxes(j_bands)\n", " remove_unneeded_fluxes(h_bands)\n", " remove_unneeded_fluxes(k_bands)\n", "\n", " cigale_input = vstack([cigale_input, best_catalogue])\n", " #best_catalogue.write(\"data_tmp/tiles/XMM-LSS_cigale_best_extcor_{}_{}.fits\".format(SUFFIX, file_num), overwrite=True)\n", " \n", " \n", "cigale_input.write(\"data_tmp/xmm-lss_cigale_optnir_extcor_{}.fits\".format(SUFFIX), overwrite=True)" ] }, { "cell_type": "markdown", "metadata": {}, "source": [ "# Catalogue using spectroscopic redshift" ] }, { "cell_type": "code", "execution_count": 15, "metadata": {}, "outputs": [ { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_60.fits:\n", "Number of good sources: 1195\n", "Number of sources with redshift in file 60: 140\n", "Tile xmm-lss_20190207_cigale_9.fits:\n", "Number of good sources: 220\n", "Number of sources with redshift in file 9: 5\n", "Tile xmm-lss_20190207_cigale_51.fits:\n", "Number of good sources: 1461\n", "Number of sources with redshift in file 51: 252\n", "Tile xmm-lss_20190207_cigale_78.fits:\n", "Number of good sources: 324\n", "Number of sources with redshift in file 78: 35\n", "Tile xmm-lss_20190207_cigale_33.fits:\n", "Number of good sources: 635\n", "Number of sources with redshift in file 33: 95\n", "Tile xmm-lss_20190207_cigale_49.fits:\n", "Number of good sources: 1149\n", "Number of sources with redshift in file 49: 189\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 1 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_55.fits:\n", "Number of good sources: 1494\n", "Number of sources with redshift in file 55: 278\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 2 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_64.fits:\n", "Number of good sources: 1215\n", "Number of sources with redshift in file 64: 82\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 2 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_37.fits:\n", "Number of good sources: 1100\n", "Number of sources with redshift in file 37: 216\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 1 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_70.fits:\n", "Number of good sources: 964\n", "Number of sources with redshift in file 70: 140\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 1 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_41.fits:\n", "Number of good sources: 1065\n", "Number of sources with redshift in file 41: 237\n", "Tile xmm-lss_20190207_cigale_23.fits:\n", "Number of good sources: 892\n", "Number of sources with redshift in file 23: 199\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 3 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_68.fits:\n", "Number of good sources: 1024\n", "Number of sources with redshift in file 68: 125\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 1 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_81.fits:\n", "Number of good sources: 38\n", "Number of sources with redshift in file 81: 2\n", "Tile xmm-lss_20190207_cigale_1.fits:\n", "Number of good sources: 0\n", "Number of sources with redshift in file 1: 0\n", "Tile xmm-lss_20190207_cigale_59.fits:\n", "Number of good sources: 1376\n", "Number of sources with redshift in file 59: 198\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 1 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_12.fits:\n", "Number of good sources: 422\n", "Number of sources with redshift in file 12: 49\n", "Tile xmm-lss_20190207_cigale_45.fits:\n", "Number of good sources: 1305\n", "Number of sources with redshift in file 45: 227\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 2 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_74.fits:\n", "Number of good sources: 669\n", "Number of sources with redshift in file 74: 112\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 1 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_5.fits:\n", "Number of good sources: 0\n", "Number of sources with redshift in file 5: 0\n", "Tile xmm-lss_20190207_cigale_16.fits:\n", "Number of good sources: 673\n", "Number of sources with redshift in file 16: 135\n", "Tile xmm-lss_20190207_cigale_27.fits:\n", "Number of good sources: 1014\n", "Number of sources with redshift in file 27: 250\n", "Tile xmm-lss_20190207_cigale_85.fits:\n", "Number of good sources: 0\n", "Number of sources with redshift in file 85: 0\n", "Tile xmm-lss_20190207_cigale_71.fits:\n", "Number of good sources: 945\n", "Number of sources with redshift in file 71: 143\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 3 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_40.fits:\n", "Number of good sources: 1119\n", "Number of sources with redshift in file 40: 252\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 1 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_69.fits:\n", "Number of good sources: 996\n", "Number of sources with redshift in file 69: 125\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 3 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_22.fits:\n", "Number of good sources: 623\n", "Number of sources with redshift in file 22: 139\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 1 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_80.fits:\n", "Number of good sources: 138\n", "Number of sources with redshift in file 80: 10\n", "Tile xmm-lss_20190207_cigale_0.fits:\n", "Number of good sources: 0\n", "Number of sources with redshift in file 0: 0\n", "Tile xmm-lss_20190207_cigale_13.fits:\n", "Number of good sources: 453\n", "Number of sources with redshift in file 13: 77\n", "Tile xmm-lss_20190207_cigale_58.fits:\n", "Number of good sources: 1442\n", "Number of sources with redshift in file 58: 228\n", "Tile xmm-lss_20190207_cigale_44.fits:\n", "Number of good sources: 1243\n", "Number of sources with redshift in file 44: 176\n", "Tile xmm-lss_20190207_cigale_75.fits:\n", "Number of good sources: 636\n", "Number of sources with redshift in file 75: 82\n", "Tile xmm-lss_20190207_cigale_4.fits:\n", "Number of good sources: 0\n", "Number of sources with redshift in file 4: 0\n", "Tile xmm-lss_20190207_cigale_17.fits:\n", "Number of good sources: 814\n", "Number of sources with redshift in file 17: 168\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 1 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_26.fits:\n", "Number of good sources: 1044\n", "Number of sources with redshift in file 26: 251\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 1 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_84.fits:\n", "Number of good sources: 0\n", "Number of sources with redshift in file 84: 0\n", "Tile xmm-lss_20190207_cigale_61.fits:\n", "Number of good sources: 1138\n", "Number of sources with redshift in file 61: 74\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 2 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_8.fits:\n", "Number of good sources: 104\n", "Number of sources with redshift in file 8: 1\n", "Tile xmm-lss_20190207_cigale_50.fits:\n", "Number of good sources: 1362\n", "Number of sources with redshift in file 50: 274\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 3 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 3 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_32.fits:\n", "Number of good sources: 882\n", "Number of sources with redshift in file 32: 165\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 2 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_79.fits:\n", "Number of good sources: 258\n", "Number of sources with redshift in file 79: 28\n", "Tile xmm-lss_20190207_cigale_48.fits:\n", "Number of good sources: 1221\n", "Number of sources with redshift in file 48: 187\n", "Tile xmm-lss_20190207_cigale_54.fits:\n", "Number of good sources: 1410\n", "Number of sources with redshift in file 54: 214\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 3 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_65.fits:\n", "Number of good sources: 1178\n", "Number of sources with redshift in file 65: 102\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 1 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_36.fits:\n", "Number of good sources: 476\n", "Number of sources with redshift in file 36: 85\n", "Tile xmm-lss_20190207_cigale_73.fits:\n", "Number of good sources: 778\n", "Number of sources with redshift in file 73: 135\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 3 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_38.fits:\n", "Number of good sources: 1106\n", "Number of sources with redshift in file 38: 235\n", "Tile xmm-lss_20190207_cigale_42.fits:\n", "Number of good sources: 1134\n", "Number of sources with redshift in file 42: 224\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 3 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_82.fits:\n", "Number of good sources: 0\n", "Number of sources with redshift in file 82: 0\n", "Tile xmm-lss_20190207_cigale_20.fits:\n", "Number of good sources: 497\n", "Number of sources with redshift in file 20: 116\n", "Tile xmm-lss_20190207_cigale_11.fits:\n", "Number of good sources: 537\n", "Number of sources with redshift in file 11: 60\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 1 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_2.fits:\n", "Number of good sources: 0\n", "Number of sources with redshift in file 2: 0\n", "Tile xmm-lss_20190207_cigale_46.fits:\n", "Number of good sources: 1254\n", "Number of sources with redshift in file 46: 246\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 1 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_77.fits:\n", "Number of good sources: 411\n", "Number of sources with redshift in file 77: 40\n", "Tile xmm-lss_20190207_cigale_15.fits:\n", "Number of good sources: 571\n", "Number of sources with redshift in file 15: 126\n", "Tile xmm-lss_20190207_cigale_6.fits:\n", "Number of good sources: 0\n", "Number of sources with redshift in file 6: 0\n", "Tile xmm-lss_20190207_cigale_86.fits:\n", "Number of good sources: 0\n", "Number of sources with redshift in file 86: 0\n", "Tile xmm-lss_20190207_cigale_24.fits:\n", "Number of good sources: 993\n", "Number of sources with redshift in file 24: 235\n", "Tile xmm-lss_20190207_cigale_28.fits:\n", "Number of good sources: 976\n", "Number of sources with redshift in file 28: 230\n", "Tile xmm-lss_20190207_cigale_63.fits:\n", "Number of good sources: 1268\n", "Number of sources with redshift in file 63: 89\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 1 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_52.fits:\n", "Number of good sources: 1384\n", "Number of sources with redshift in file 52: 204\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 1 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_19.fits:\n", "Number of good sources: 645\n", "Number of sources with redshift in file 19: 125\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 2 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_30.fits:\n", "Number of good sources: 965\n", "Number of sources with redshift in file 30: 222\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 1 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_56.fits:\n", "Number of good sources: 1380\n", "Number of sources with redshift in file 56: 246\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 3 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_67.fits:\n", "Number of good sources: 1136\n", "Number of sources with redshift in file 67: 104\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 1 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_34.fits:\n", "Number of good sources: 787\n", "Number of sources with redshift in file 34: 152\n", "Tile xmm-lss_20190207_cigale_62.fits:\n", "Number of good sources: 1312\n", "Number of sources with redshift in file 62: 100\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 1 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_29.fits:\n", "Number of good sources: 898\n", "Number of sources with redshift in file 29: 212\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 1 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_18.fits:\n", "Number of good sources: 930\n", "Number of sources with redshift in file 18: 200\n", "Tile xmm-lss_20190207_cigale_53.fits:\n", "Number of good sources: 1394\n", "Number of sources with redshift in file 53: 215\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 1 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_31.fits:\n", "Number of good sources: 862\n", "Number of sources with redshift in file 31: 206\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 1 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_57.fits:\n", "Number of good sources: 1339\n", "Number of sources with redshift in file 57: 209\n", "Tile xmm-lss_20190207_cigale_66.fits:\n", "Number of good sources: 1143\n", "Number of sources with redshift in file 66: 113\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 2 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_35.fits:\n", "Number of good sources: 625\n", "Number of sources with redshift in file 35: 117\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 2 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_39.fits:\n", "Number of good sources: 1201\n", "Number of sources with redshift in file 39: 220\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 1 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_72.fits:\n", "Number of good sources: 917\n", "Number of sources with redshift in file 72: 150\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 4 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 2 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_43.fits:\n", "Number of good sources: 1197\n", "Number of sources with redshift in file 43: 227\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 1 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_83.fits:\n", "Number of good sources: 0\n", "Number of sources with redshift in file 83: 0\n", "Tile xmm-lss_20190207_cigale_21.fits:\n", "Number of good sources: 723\n", "Number of sources with redshift in file 21: 149\n", "Tile xmm-lss_20190207_cigale_10.fits:\n", "Number of good sources: 390\n", "Number of sources with redshift in file 10: 32\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 1 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_3.fits:\n", "Number of good sources: 0\n", "Number of sources with redshift in file 3: 0\n", "Tile xmm-lss_20190207_cigale_47.fits:\n", "Number of good sources: 1270\n", "Number of sources with redshift in file 47: 240\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 2 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_76.fits:\n", "Number of good sources: 589\n", "Number of sources with redshift in file 76: 75\n", "Tile xmm-lss_20190207_cigale_14.fits:\n", "Number of good sources: 505\n", "Number of sources with redshift in file 14: 80\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 3 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] }, { "name": "stdout", "output_type": "stream", "text": [ "Tile xmm-lss_20190207_cigale_7.fits:\n", "Number of good sources: 13\n", "Number of sources with redshift in file 7: 0\n", "Tile xmm-lss_20190207_cigale_87.fits:\n", "Number of good sources: 0\n", "Number of sources with redshift in file 87: 0\n", "Tile xmm-lss_20190207_cigale_25.fits:\n", "Number of good sources: 1055\n", "Number of sources with redshift in file 25: 252\n" ] }, { "name": "stderr", "output_type": "stream", "text": [ "INFO:herschelhelp.external:For 4 sources, the band megacam_u should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 4 sources, the band suprime_b should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band decam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band megacam_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band gpc1_g should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band suprime_v should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n", "INFO:herschelhelp.external:For 1 sources, the band acs_f606w should not be used because it overlaps or is below the Lyman limit at the redshift of these sources. These fluxes were set to NaN.\n" ] } ], "source": [ "cigale_input = Table()\n", "\n", "for tile in file_list:\n", " \n", " file_num = tile.split('_')[4].split('.')[0]\n", " print(\"Tile {}:\".format(tile.split('/')[-1]))\n", " best_catalogue = Table.read(tile)\n", " best_catalogue = main_help_sample(best_catalogue)\n", " \n", " optnir = ((best_catalogue['flag_optnir_det'] == 3) \n", " | (best_catalogue['flag_optnir_det'] == 7))\n", " \n", " best_catalogue = best_catalogue[optnir]\n", "\n", " best_catalogue.remove_column(\"redshift\")\n", " best_catalogue[\"zspec\"].name = \"redshift\"\n", " best_catalogue = best_catalogue[~np.isnan(best_catalogue[\"redshift\"])]\n", "\n", " print(\"Number of sources with redshift in file {}: {}\".format(file_num, len(best_catalogue)))\n", "\n", " # Correction for galactic extinction\n", " best_catalogue = correct_galactic_extinction(best_catalogue, inplace=True)\n", "\n", " # Convertion to CIGALE format\n", "\n", " best_catalogue = convert_table_for_cigale(best_catalogue, inplace=True, remove_zerofluxes=True)\n", "\n", " remove_unneeded_fluxes(g_bands)\n", " remove_unneeded_fluxes(u_bands)\n", " remove_unneeded_fluxes(r_bands)\n", " remove_unneeded_fluxes(i_bands)\n", " remove_unneeded_fluxes(z_bands)\n", " remove_unneeded_fluxes(y_bands)\n", " remove_unneeded_fluxes(j_bands)\n", " remove_unneeded_fluxes(h_bands)\n", " remove_unneeded_fluxes(k_bands)\n", "\n", " cigale_input = vstack([cigale_input, best_catalogue])\n", " #best_catalogue.write(\"data_tmp/tiles/XMM-LSS_cigale_best_extcor_{}_{}.fits\".format(SUFFIX, file_num), overwrite=True)\n", " \n", " \n", "cigale_input.write(\"data_tmp/xmm-lss_cigale_optnir_extcor_zspec_{}.fits\".format(SUFFIX), overwrite=True)" ] } ], "metadata": { "kernelspec": { "display_name": "Python (herschelhelp_internal)", "language": "python", "name": "helpint" }, "language_info": { "codemirror_mode": { "name": "ipython", "version": 3 }, "file_extension": ".py", "mimetype": "text/x-python", "name": "python", "nbconvert_exporter": "python", "pygments_lexer": "ipython3", "version": "3.7.2" } }, "nbformat": 4, "nbformat_minor": 2 }