{
"cells": [
{
"cell_type": "markdown",
"metadata": {},
"source": [
"# Make VO table of extreme starbursts\n",
"\n",
"Reprocessing the manually made csv file from https://docs.google.com/spreadsheets/d/1hF9ls8AMzzY--2I5tukqBmJf6xf7LO8lB4NTr3sFu08/edit#gid=0"
]
},
{
"cell_type": "code",
"execution_count": 1,
"metadata": {},
"outputs": [],
"source": [
"from astropy.table import Table, Column\n",
"from astropy.coordinates import SkyCoord\n",
"\n",
"import numpy as np\n",
"\n",
"import yaml\n",
"\n",
"from pymoc import MOC\n",
"\n",
"from herschelhelp_internal.utils import coords_to_hpidx, gen_help_id, inMoc"
]
},
{
"cell_type": "code",
"execution_count": 2,
"metadata": {},
"outputs": [],
"source": [
"giants = Table.read('./data/Known_Monsters_Sheet1.csv')"
]
},
{
"cell_type": "code",
"execution_count": 3,
"metadata": {},
"outputs": [
{
"data": {
"text/html": [
"Table masked=True length=130\n",
"
\n",
"Name | RA | Dec | Redshift | Redshift source | Lbol/Lsun intrinsic | Lensed? | Original survey | Reference | Notes |
\n",
"str24 | str22 | str13 | str10 | str14 | str11 | str9 | str17 | str106 | str152 |
\n",
"9io9 | 02h09m41.3s | 00d15m58.6s | 2.553 | CO, H-alpha | 1.00E+13 | Y mu~10 | Planck/ACT/VICS82 | http://adsabs.harvard.edu/abs/2015MNRAS.452..502G | -- |
\n",
"WISE J132934.18+224327.3 | 13h29m34.18s | 22d43m27.3s | 2.0439 | H-alpha | 1.30E+13 | Y mu~11 | WISE/Planck | http://adsabs.harvard.edu/abs/2017ApJ...843L..22D | -- |
\n",
"Orochi | 02h18m30.7s | -05d31m31s | 3.4 | CO | ~1.30e13 | Y mu~5 | AzTEC-ASTE | http://adsabs.harvard.edu/abs/2011MNRAS.415.3081I | -- |
\n",
"MMJ154506.4−344318 | 15h45m06.35s | -34d43m18.2s | 04-May | est | >1e13 | ? | AzTEC-ASTE | http://adsabs.harvard.edu/abs/2015ApJ...808..121T | -- |
\n",
"MMJ154132.7−350320 | 15h41m32.71s | -35d03m23.3s | 3 | est | 13.7-13.9 | Y mu~1.2 | AzTEC-ASTE | http://adsabs.harvard.edu/abs/2015ApJ...808..121T | -- |
\n",
"GN20 | 12h37m12s | 62d22m12.100s | 4.06 | CO | 2.90E+13 | N | GOODS-N | http://adsabs.harvard.edu/abs/2009ApJ...694.1517D | -- |
\n",
"SPT0103-45 | 15.797917 | -45.648306 | 3.0917 | ALMA 3mm CO | 1.67E+13 | mu = 5.34 | SPT-SZ | https://ui.adsabs.harvard.edu/#abs/2016ApJ...826..112S/abstract | Contact: jspilker@utexas.edu |
\n",
"SPT0125-47 | 21.2795 | -47.398889 | 2.5148 | ALMA 3mm CO | 3.33E+13 | mu = 5.47 | SPT-SZ | https://ui.adsabs.harvard.edu/#abs/2016ApJ...826..112S/abstract | Contact: jspilker@utexas.edu |
\n",
"SPT0243-49 | 40.786708 | -46.35675 | 5.699 | ALMA 3mm CO | 1.63E+13 | mu = 5.09 | SPT-SZ | https://ui.adsabs.harvard.edu/#abs/2016ApJ...826..112S/abstract | Contact: jspilker@utexas.edu |
\n",
"SPT0300-46 | 45.018208 | -46.35675 | 3.5954 | ALMA 3mm CO | 1.26E+13 | mu = 6.30 | SPT-SZ | https://ui.adsabs.harvard.edu/#abs/2016ApJ...826..112S/abstract | Contact: jspilker@utexas.edu |
\n",
"... | ... | ... | ... | ... | ... | ... | ... | ... | ... |
\n",
"-- | 138.158467 | 2.01306424 | 3.04128003 | spec-z | 1.32E+13 | -- | HELP | https://github.com/StevenDuivenvoorden/FIR-group/blob/master/Ian/plotting_tools/HELP_ULIRG_selection.ipynb | Sources selected from the HELP databse using the code on GITHUB |
\n",
"-- | 9.17275683 | -43.343878 | 0.13801 | spec-z | 1.99E+13 | -- | HELP | https://github.com/StevenDuivenvoorden/FIR-group/blob/master/Ian/plotting_tools/HELP_ULIRG_selection.ipynb | Sources selected from the HELP databse using the code on GITHUB |
\n",
"-- | 8.32921426 | -45.388595 | 0.13500001 | spec-z | 1.12E+13 | -- | HELP | https://github.com/StevenDuivenvoorden/FIR-group/blob/master/Ian/plotting_tools/HELP_ULIRG_selection.ipynb | Sources selected from the HELP databse using the code on GITHUB |
\n",
"-- | 8.68245338 | -45.189448 | 0.57800001 | spec-z | 1.39E+13 | -- | HELP | https://github.com/StevenDuivenvoorden/FIR-group/blob/master/Ian/plotting_tools/HELP_ULIRG_selection.ipynb | Sources selected from the HELP databse using the code on GITHUB |
\n",
"-- | 242.824989 | 54.3402405 | 0.59622699 | spec-z | 2.30E+13 | -- | HELP | https://github.com/StevenDuivenvoorden/FIR-group/blob/master/Ian/plotting_tools/HELP_ULIRG_selection.ipynb | Sources selected from the HELP databse using the code on GITHUB |
\n",
"-- | 240.811248 | 54.3738727 | 1.75600004 | spec-z | 1.37E+13 | -- | HELP | https://github.com/StevenDuivenvoorden/FIR-group/blob/master/Ian/plotting_tools/HELP_ULIRG_selection.ipynb | Sources selected from the HELP databse using the code on GITHUB |
\n",
"-- | 245.194985 | 55.4695492 | 0.60170501 | spec-z | 1.78E+13 | -- | HELP | https://github.com/StevenDuivenvoorden/FIR-group/blob/master/Ian/plotting_tools/HELP_ULIRG_selection.ipynb | Sources selected from the HELP databse using the code on GITHUB |
\n",
"-- | 242.830416 | 56.5343897 | 3.49065995 | spec-z | 1.56E+13 | -- | HELP | https://github.com/StevenDuivenvoorden/FIR-group/blob/master/Ian/plotting_tools/HELP_ULIRG_selection.ipynb | Sources selected from the HELP databse using the code on GITHUB |
\n",
"-- | 241.414947 | 54.7630619 | 2.44812989 | spec-z | 1.24E+13 | -- | HELP | https://github.com/StevenDuivenvoorden/FIR-group/blob/master/Ian/plotting_tools/HELP_ULIRG_selection.ipynb | Sources selected from the HELP databse using the code on GITHUB |
\n",
"-- | -- | -- | -- | phot-z | -- | -- | HELP | https://github.com/StevenDuivenvoorden/FIR-group/blob/master/Ian/plotting_tools/HELP_ULIRG_selection.ipynb | There are an additional ~1900 sources whose solar luminosity is >10^13 solar luminosities in the HELP databse but which only have photometric redshifts. |
\n",
"
"
],
"text/plain": [
"