# Master list on XMM-LSS This folder contains the Jupyter notebooks used to create HELP mater list on XMM-LSS. | Survey | Telescope / Instrument | Filters (detection band in bold) | Location | |--------|-------------------------|:---------------------------------:|-----------------| | CANDELS-3D-HST | HST | F140W, F160W, F606W, F814W, F125W | dmu0_CANDELS-3D-HST | | CANDELS-UDS | HST | ACS_F435W, ACS_F606W, ACS_F775W, ACS_F814W, ACS_F850LP, WFC3_F098M, WFC3_F105W, WFC3_F125W, WFC3_F140W, WFC3_F160W | dmu0_CANDELS-UDS | | CFHT-WIRDS | CFHT | J, H, Ks | dmu0_CFHT-WIRDS | | CFHTLS | CFHT | u*, g', r', i', z' | dmu0_CFHTLS | | CFHTLenS | CFHT | u, g, r, i, z | dmu0_CFHTLenS | | DECaLS | DEC | ugrizY | dmu0_DECaLS | | SERVS | Spitzer | IRAC1234, MIPS123 |mu0_DataFusion-Spitzer | | SWIRE | Spitzer | IRAC1234, MIPS123 |mu0_DataFusion-Spitzer | | HSC-SSP | Subaru/Suprime | grizy | dmu0_HSC | | PanSTARRS-3SS | GPC1 | grizy | dmu0_PanSTARRS1-3SS | | SXDS | Subaru/Suprime | B, V, r, i, z | dmu0_SXDS | | SpARCS | CFHT | u, g, r, y, z | dmu0_SpARCS | | UKIDSS-DXS | UKIRT WFCAM | YJHK? | dmu0_UKIDSS-DXS_DR10plus | | UKIDSS-UDS | UKIRT WFCAM | YJHK? | dmu0_UKIDSS-UDS | | VIPERS | ZYHJKs? | dmu0_VIPERS-MLS | | VHS | VISTA VIRCAM | ZYHJKs? | dmu0_VISTA-VHS | | VIDEO | VISTA VIRCAM | ZYHJKs? | dmu0_VISTA-VIDEO-private | | VIKING | VISTA VIRCAM | ZYHJKs | dmu0_VISTA-VIKING | | DES | Blanco/DECam | grizy | dmu0_DES | ## Pristine catalogue preparations For each pristine catalogue, a specific notebook is used for its preparation: the selection of columns, the conversion of some magnitudes or fluxes when needed, the removal of duplicated sources, the correction of astrometry using Gaia as reference, and the flagging of possible Gaia objects. - [1.1_CANDELS-3D-HST.ipynb](1.1_CANDELS-3D-HST.ipynb) - [1.2_CANDELS-UDS.ipynb](1.2) - [1.3_CFHT-WIRDS.ipynb](1.3_CFHT-WIRDS.ipynb) - [1.4.1_CFHTLS-WIDE.ipynb](1.4.1_CFHTLS-WIDE.ipynb) - [1.4.2_CFHTLS-WIDE.ipynb](1.4.2_CFHTLS-WIDE.ipynb) - [1.5_CFHTLenS.ipynb](1.5_CFHTLenS.ipynb) - [1.6.1_DECaLS.ipynb](1.6.1_DECaLS.ipynb) - [1.6.2_DES.ipynb](1.6.2_DES.ipynb) - [1.7_SWIRE.ipynb](1.7_SWIRE.ipynb) - [1.8_SERVS.ipynb](1.8_SERVS.ipynb) - [1.9.1_HSC-WIDE.ipynb](1.9.1_HSC-WIDE.ipynb) - [1.9.2_HSC-DEEP.ipynb](1.9.2_HSC-DEEP.ipynb) - [1.9.3_HSC-UDEEP.ipynb](1.9.3_HSC-UDEEP.ipynb) - [1.10_PanSTARRS1-3SS.ipynb](1.10_PanSTARRS1-3SS.ipynb) - [1.11_SXDS.ipynb](1.11_) - [1.12_SpARCS.ipynb](1.12_SpARCS.ipynb) - [1.13_UKIDSS-DXS.ipynb](1.13_UKIDSS-DXS.ipynb) - [1.14_UKIDSS-UDS.ipynb](1.14_UKIDSS-UDS.ipynb) - [1.15_VIPERS.ipynb](1.15_VIPERS.ipynb) - [1.17_VISTA-VIDEO.ipynb](1.17_VISTA-VIDEO.ipynb) - [1.18_VISTA-VIKING.ipynb](1.18_VISTA-VIKING.ipynb) ## Catalogue merging The merging notebooks performs the merging of the pristine catalogues into the master list. Because XMM-LSS has so much data we must merge the similar bands first and then do the final merge on tiles as for HS82 and SGP. THe final stage is then to concatenate the tables using Stilts. - [2.1_Megacam_merge.ipynb](2.1_Megacam_merge.ipynb) - [2.2_UKIDSS_merge.ipynb](2.2_UKIDSS_merge.ipynb) - [2.3_HSC_merge.ipynb](2.3_HSC_merge.ipynb) - [2.4_VISTA_merge.ipynb](2.4_VISTA_merge.ipynb) - [2.5_IRAC_merge.ipynb](2.5_IRAC_merge.ipynb) - [2.6_DECAM_merging.ipynb](2.6_DECAM_merging.ipynb) - [2.7_Merging.ipynb](2.7_Merging.ipynb) ## Diagnostics The [3_Checks_and_diagnostics.ipynb](3_Checks_and_diagnostics.ipynb) notebook presents some checks and diagnostic plots on the final master list.