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Table: ls_dr6.dr6_superset_dr12q
(The bold columns are indexed columns)
| Column Name | Description | Datatype |
|---|
Astro Data Lab
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datalab.noirlab.edu/tap
- allwise
- allwise.sourceAllWISE Source Table (747M objects)
- allwise.x1p5__source__catwise2020__mainxmatch_std.allwise__source and catwise2020.main crossmatch (1.5 arcsec)
- allwise.x1p5__source__decaps_dr1__objectallwise.source and decaps_dr1.object crossmatch (1.5 arcsec)
- allwise.x1p5__source__decaps_dr2__objectxmatch_std.allwise__source and decaps_dr2.object crossmatch (1.5 arcsec)
- allwise.x1p5__source__delve_dr1__objectsallwise.source and delve_dr1.objects crossmatch (1.5 arcsec)
- allwise.x1p5__source__delve_dr2__objectsxmatch_std.allwise__source and delve_dr2.objects crossmatch (1.5 arcsec)
- allwise.x1p5__source__des_dr1__mainallwise.source and des_dr1.main crossmatch (1.5 arcsec)
- allwise.x1p5__source__des_dr2__mainxmatch_std.allwise__source and xmatch_std.des_dr2__main crossmatch (1.5 arcsec)
- allwise.x1p5__source__desi_edr__zpixxmatch_std.allwise__source and desi_edr.zpix crossmatch (1.5 arcsec)
- allwise.x1p5__source__gaia_dr1__gaia_sourceallwise.source and gaia_dr1.gaia_source crossmatch (1.5 arcsec)
- allwise.x1p5__source__gaia_dr2__gaia_sourceallwise.source and gaia_dr2.gaia_source crossmatch (1.5 arcsec)
- allwise.x1p5__source__gaia_dr3__gaia_sourcexmatch_std.allwise__source and gaia_dr3.gaia_source crossmatch (1.5 arcsec)
- allwise.x1p5__source__gnirs_dqs__spec_measurementsxmatch_std.allwise__source and gnirs_dqs.spec_measurements crossmatch (1.5 arcsec)
- allwise.x1p5__source__gogreen_dr1__photoallwise.source and gogreen_dr1.photo crossmatch (1.5 arcsec)
- allwise.x1p5__source__gogreen_dr1__redshiftallwise.source and gogreen_dr1.redshift crossmatch (1.5 arcsec)
- allwise.x1p5__source__ls_dr10__tractorxmatch_std.allwise__source and ls_dr10.tractor crossmatch (1.5 arcsec)
- allwise.x1p5__source__ls_dr8__tractorxmatch_std.allwise__source and ls_dr8.tractor crossmatch (1.5 arcsec)
- allwise.x1p5__source__ls_dr9__tractorxmatch_std.allwise__source and xmatch_std.ls_dr9__tractor crossmatch (1.5 arcsec)
- allwise.x1p5__source__nsc_dr2__objectallwise.source and nsc_dr2.object crossmatch (1.5 arcsec)
- allwise.x1p5__source__phat_v2__phot_modallwise.source and phat_v2.phot_mod crossmatch (1.5 arcsec)
- allwise.x1p5__source__sdss_dr12__specobjallwise.source and sdss_dr12.specobj crossmatch (1.5 arcsec)
- allwise.x1p5__source__sdss_dr13__specobjallwise.source and sdss_dr13.specobj crossmatch (1.5 arcsec)
- allwise.x1p5__source__sdss_dr14__specobjallwise.source and sdss_dr14.specobj crossmatch (1.5 arcsec)
- allwise.x1p5__source__sdss_dr16__specobjallwise.source and sdss_dr16.specobj crossmatch (1.5 arcsec)
- allwise.x1p5__source__sdss_dr17__specobjxmatch_std.allwise__source and sdss_dr17.specobj crossmatch (1.5 arcsec)
- allwise.x1p5__source__sga2020__tractorxmatch_std.allwise__source and sga2020.tractor crossmatch (1.5 arcsec)
- allwise.x1p5__source__skymapper_dr1__masterallwise.source and skymapper_dr1.master crossmatch (1.5 arcsec)
- allwise.x1p5__source__skymapper_dr2__masterxmatch_std.allwise__source and xmatch_std.skymapper_dr2__master crossmatch (1.5 arcsec)
- allwise.x1p5__source__smash_dr1__objectallwise.source and smash_dr1.object crossmatch (1.5 arcsec)
- allwise.x1p5__source__smash_dr2__objectallwise.source and smash_dr2.object crossmatch (1.5 arcsec)
- allwise.x1p5__source__splus_dr1__stripe82allwise.source and splus_dr1.stripe82 crossmatch (1.5 arcsec)
- allwise.x1p5__source__splus_dr2__mainxmatch_std.allwise__source and xmatch_std.splus_dr2__main crossmatch (1.5 arcsec)
- allwise.x1p5__source__splus_edr__stripe82allwise.source and splus_edr.stripe82 crossmatch (1.5 arcsec)
- allwise.x1p5__source__twomass__pscallwise.source and twomass.psc crossmatch (1.5 arcsec)
- allwise.x1p5__source__twomass__xscallwise.source and twomass.xsc crossmatch (1.5 arcsec)
- allwise.x1p5__source__tycho2__mainallwise.source and tycho2.main crossmatch (1.5 arcsec)
- allwise.x1p5__source__ukidss_dr11plus__dxssourcexmatch_std.allwise__source and ukidss_dr11plus.dxssource crossmatch (1.5 arcsec)
- allwise.x1p5__source__ukidss_dr11plus__gcssourcexmatch_std.allwise__source and ukidss_dr11plus.gcssource crossmatch (1.5 arcsec)
- allwise.x1p5__source__ukidss_dr11plus__gpssourcexmatch_std.allwise__source and ukidss_dr11plus.gpssource crossmatch (1.5 arcsec)
- allwise.x1p5__source__ukidss_dr11plus__lassourcexmatch_std.allwise__source and ukidss_dr11plus.lassource crossmatch (1.5 arcsec)
- allwise.x1p5__source__ukidss_dr11plus__udssourcexmatch_std.allwise__source and ukidss_dr11plus.udssource crossmatch (1.5 arcsec)
- allwise.x1p5__source__unwise_dr1__objectallwise.source and unwise_dr1.object crossmatch (1.5 arcsec)
- allwise.x1p5__source__usno__a2allwise.source and usno.a2 crossmatch (1.5 arcsec)
- allwise.x1p5__source__usno__b1allwise.source and usno.b1 crossmatch (1.5 arcsec)
- allwise.x1p5__source__vhs_dr5__vhs_cat_v3allwise.source and vhs_dr5.vhs_cat_v3 crossmatch (1.5 arcsec)
- buzzard_dr1
- catwise2020
- catwise2020.mainCatWise2020 Main Table. For more details on the columns, see https://portal.nersc.gov/project/cosmo/data/CatWISE/2020cwcat.sis20200318.txt
- catwise2020.x1p5__main__allwise__sourcecatwise2020.main and xmatch_std.allwise__source crossmatch (1.5 arcsec)
- catwise2020.x1p5__main__gaia_dr3__gaia_sourcecatwise2020.main and xmatch_std.gaia_dr3__gaia_source crossmatch (1.5 arcsec)
- catwise2020.x1p5__main__nsc_dr2__objectcatwise2020.main and xmatch_std.nsc_dr2__object crossmatch (1.5 arcsec)
- catwise2020.x1p5__main__sdss_dr17__specobjcatwise2020.main and xmatch_std.sdss_dr17__specobj crossmatch (1.5 arcsec)
- catwise2020.x1p5__main__unwise_dr1__objectcatwise2020.main and xmatch_std.unwise_dr1__object crossmatch (1.5 arcsec)
- dad_dr1
- dad_dr1.movdsThis table describes the characteristics of the datasets (pointings). The time and position fields are for the start of the first observation exposure in the set. Position fields are for the center of the field.
- dad_dr1.movdup
- dad_dr1.movexpThe exposure table provides details of each exposure. The expname is a way to link to the image data in the NOIRLab Science Archive. The expid is the sequencial count of the exposures in a dataset. The separation time is a relative time for the middle of each exposure with an origin at the start of the first exposure.
- dad_dr1.movgrpThis is the main tracklet table. It provides information about each connected set of observations corresponding to a moving object.
- dad_dr1.movmpcThe MPC records are basically an encoding of the information in the exposure and observation tables in a specific format for reporting the time, position, and estimated magnitude for an observation.
- dad_dr1.movobsThese tables provide information for each separate detection of a moving object. They provide links to associated files (see below) and to what was reported to the MPC.
- dad_dr1.movrate
- dad_dr2
- dad_dr2.addgrp
- dad_dr2.addobs
- dad_dr2.movdsThis table describes the characteristics of the datasets (pointings). The time and position fields are for the start of the first observation exposure in the set. Position fields are for the center of the field.
- dad_dr2.movdup
- dad_dr2.movexpThe exposure table provides details of each exposure. The expname is a way to link to the image data in the NOIRLab Science Archive. The expid is the sequencial count of the exposures in a dataset. The separation time is a relative time for the middle of each exposure with an origin at the start of the first exposure.
- dad_dr2.movgrpThis is the main tracklet table. It provides information about each connected set of observations corresponding to a moving object.
- dad_dr2.movmpcThe MPC records are basically an encoding of the information in the exposure and observation tables in a specific format for reporting the time, position, and estimated magnitude for an observation.
- dad_dr2.movobsThese tables provide information for each separate detection of a moving object. They provide links to associated files (see below) and to what was reported to the MPC.
- dad_dr2.movrate
- decaps_dr1
- decaps_dr1.ccdsBrick CCD table
- decaps_dr1.depthBrick depth table
- decaps_dr1.imdbImage header table
- decaps_dr1.measMeasurement table
- decaps_dr1.objectBand-merged catalog
- decaps_dr1.x1p5__object__allwise__sourcedecaps_dr1.object and allwise.source crossmatch (1.5 arcsec)
- decaps_dr1.x1p5__object__gaia_dr3__gaia_sourcexmatch_std.decaps_dr1__object and gaia_dr3.gaia_source crossmatch (1.5 arcsec)
- decaps_dr1.x1p5__object__nsc_dr2__objectdecaps_dr1.object and nsc_dr2.object crossmatch (1.5 arcsec)
- decaps_dr1.x1p5__object__sdss_dr17__specobjxmatch_std.decaps_dr1__object and sdss_dr17.specobj crossmatch (1.5 arcsec)
- decaps_dr1.x1p5__object__unwise_dr1__objectdecaps_dr1.object and unwise_dr1.object crossmatch (1.5 arcsec)
- decaps_dr1.zpsZero points, flat fields, & QA table
- decaps_dr2
- decaps_dr2.objectBand-merged calibrated object catalog
- decaps_dr2.x1p5__object__allwise__sourcedecaps_dr2.object and xmatch_std.allwise__source crossmatch (1.5 arcsec)
- decaps_dr2.x1p5__object__gaia_dr3__gaia_sourcedecaps_dr2.object and gaia_dr3.gaia_source crossmatch (1.5 arcsec)
- decaps_dr2.x1p5__object__nsc_dr2__objectdecaps_dr2.object and xmatch_std.nsc_dr2__object crossmatch (1.5 arcsec)
- decaps_dr2.x1p5__object__sdss_dr17__specobjdecaps_dr2.object and sdss_dr17.specobj crossmatch (1.5 arcsec)
- decaps_dr2.x1p5__object__unwise_dr1__objectdecaps_dr2.object and xmatch_std.unwise_dr1__object crossmatch (1.5 arcsec)
- delve_dr1
- delve_dr1.objectsMain DELVE DR1 object table
- delve_dr1.x1p5__objects__allwise__sourcedelve_dr1.objects and allwise.source crossmatch (1.5 arcsec)
- delve_dr1.x1p5__objects__gaia_dr3__gaia_sourcedelve_dr1.objects and gaia_dr3.gaia_source crossmatch (1.5 arcsec)
- delve_dr1.x1p5__objects__nsc_dr2__objectdelve_dr1.objects and nsc_dr2.object crossmatch (1.5 arcsec)
- delve_dr1.x1p5__objects__sdss_dr17__specobjdelve_dr1.objects and sdss_dr17.specobj crossmatch (1.5 arcsec)
- delve_dr1.x1p5__objects__unwise_dr1__objectdelve_dr1.objects and unwise_dr1.object crossmatch (1.5 arcsec)
- delve_dr2
- delve_dr2.objectsMain DELVE DR2 object table
- delve_dr2.photozValue-Added Catalog of photometric redshifts built using a Mixture Density Network trained on griz mags and colors of DELVE DR2
- delve_dr2.x1p5__objects__allwise__sourcedelve_dr2.objects and xmatch_std.allwise__source crossmatch (1.5 arcsec)
- delve_dr2.x1p5__objects__gaia_dr3__gaia_sourcedelve_dr2.objects and gaia_dr3.gaia_source crossmatch (1.5 arcsec)
- delve_dr2.x1p5__objects__nsc_dr2__objectdelve_dr2.objects and xmatch_std.nsc_dr2__object crossmatch (1.5 arcsec)
- delve_dr2.x1p5__objects__sdss_dr17__specobjdelve_dr2.objects and sdss_dr17.specobj crossmatch (1.5 arcsec)
- delve_dr2.x1p5__objects__unwise_dr1__objectdelve_dr2.objects and xmatch_std.unwise_dr1__object crossmatch (1.5 arcsec)
- des_dr1
- des_dr1.baosampleDES_Y1A1_LSSBAO_v1.1_CATALOG.fits. Main BAO sample catalog detailed in Crocce et al. (2018)
- des_dr1.des_galexGALEX (AIS) 1-arcsec xmatch v. DES
- des_dr1.des_hsc2HSC2 1-arcsec xmatch v. DES
- des_dr1.des_simbadSIMBAD 1-arcsec xmatch v. DES
- des_dr1.fluxObject flux table
- des_dr1.galaxiesGalaxies in DES
- des_dr1.im3shapeGalaxy shape catalogues using a maximum-likelihood bulge/disc model calibrated using simulations, applied to r-band data, yielding 21.9M objects
- des_dr1.img2coaddImages contributing to coadded tiles
- des_dr1.magObject magnitude table
- des_dr1.mainMain object table
- des_dr1.mockGalaxy mock catalogues of the Baryonic Acoustic Oscillation (BAO) angular distance using only photometry (for details, see https://ui.adsabs.harvard.edu/abs/2018MNRAS.479...94A/abstract)
- des_dr1.mofMulti-Object Fitting (MOF) Catalogs (for details, see https://des.ncsa.illinois.edu/releases/y1a1/key-catalogs/key-mof)
- des_dr1.morphMorphology Catalog (for details, see https://des.ncsa.illinois.edu/releases/y1a1/gold/morphology)
- des_dr1.photo_zPhotometric redshifts catalog (for details, see https://des.ncsa.illinois.edu/releases/y1a1/key-catalogs/key-photoz)
- des_dr1.psfPoint spread function catalog (for details, see https://des.ncsa.illinois.edu/releases/y1a1/key-catalogs/key-psf)
- des_dr1.sgsep_cosmos_tests_v2Star-galaxy separation catalog, covering DES observations from the Science Verification period and other DECam observations over the COSMOS field (for more details, see https://des.ncsa.illinois.edu/releases/y1a1/gold/classification)
- des_dr1.sgsep_hsc_tests_v2Star-galaxy separation catalog, covering DES observations from the Science Verification period over two specific fields with Hubble Space Telescope observations (downloaded from the https://archive.stsci.edu/hst/hsc/ site) with the ACS camera (other than COSMOS) appropriate for star-galaxy separation tests (for more details, see https://des.ncsa.illinois.edu/releases/y1a1/gold/classification)
- des_dr1.sgsep_stripe82_tests_v2Star-galaxy separation catalog, covering stripe 82 observations from SDSS with DES Y1 data (for more details, see https://des.ncsa.illinois.edu/releases/y1a1/gold/classification)
- des_dr1.sgsep_validation_masked_v3Star-galaxy separation catalog, covering This file covers observations in the main Y1 footprint with selected columns from Gold, MOF, photo-z and star-galaxy classifiers (for more details, see https://des.ncsa.illinois.edu/releases/y1a1/gold/classification)
- des_dr1.sgsep_vvds_tests_v2Star-galaxy separation catalog, voering VVDS observations with DES from the Science Verification period (for more details, see https://des.ncsa.illinois.edu/releases/y1a1/gold/classification)
- des_dr1.shape_metacal_flux_grizGalaxy shape catalogues using a Gaussian model with an innovative internal calibration scheme, applied to riz-bands, yielding 34.8M objects
- des_dr1.shape_metacal_riz_unblindGalaxy shape catalogues using a Gaussian model with an innovative internal calibration scheme, applied to riz-bands, yielding 34.8M objects
- des_dr1.tile_infoSurvey tile information table
- des_dr1.x1p5__main__allwise__sourcedes_dr1.main and allwise.source crossmatch (1.5 arcsec)
- des_dr1.x1p5__main__gaia_dr3__gaia_sourcedes_dr1.main and gaia_dr3.gaia_source crossmatch (1.5 arcsec)
- des_dr1.x1p5__main__nsc_dr2__objectdes_dr1.main and nsc_dr2.object crossmatch (1.5 arcsec)
- des_dr1.x1p5__main__sdss_dr17__specobjdes_dr1.main and sdss_dr17.specobj crossmatch (1.5 arcsec)
- des_dr1.x1p5__main__unwise_dr1__objectdes_dr1.main and unwise_dr1.object crossmatch (1.5 arcsec)
- des_dr1.y3_goldDark Energy Survey Year 3 - Cosmology Photometric Data Set
- des_dr1.y3_gold_footprintDark Energy Survey Year 3 - Cosmology Photometric Data Set, Foot Print
- des_dr1.y3_gold_surveyconditionsDark Energy Survey Year 3 - Cosmology Photometric Data Set, Survey Conditions
- des_dr2
- des_dr2.coverageSurvey coverage table
- des_dr2.fluxObject flux table
- des_dr2.magObject magnitude table
- des_dr2.mainMain object table
- des_dr2.x1p5__main__allwise__sourcexmatch_std.des_dr2__main and xmatch_std.allwise__source crossmatch (1.5 arcsec)
- des_dr2.x1p5__main__gaia_dr3__gaia_sourcexmatch_std.des_dr2__main and gaia_dr3.gaia_source crossmatch (1.5 arcsec)
- des_dr2.x1p5__main__nsc_dr2__objectdes_dr2.main and nsc_dr2.object crossmatch (1.5 arcsec)
- des_dr2.x1p5__main__sdss_dr17__specobjxmatch_std.des_dr2__main and sdss_dr17.specobj crossmatch (1.5 arcsec)
- des_dr2.x1p5__main__unwise_dr1__objectdes_dr2.main and unwise_dr1.object crossmatch (1.5 arcsec)
- des_sva1
- des_sva1.gold_annz2_pdfThe PDFs have the following binning in redshift: z_min = 0.00, z_max = 1.8, nbins = 180
- des_sva1.gold_annz2_pointThe structure of the point estimate files are identical. They each contain two columns: the SVA1 unique object identifier and the mean photo-z for that object.
- des_sva1.gold_bpz_pdfThe PDFs have the following binning in redshift: z_min = 0.005, z_max = 2.505 , nbins = 250
- des_sva1.gold_bpz_pointThe structure of the point estimate files are identical. They each contain two columns: the SVA1 unique object identifier and the mean photo-z for that object.
- des_sva1.gold_catalogThe SVA1 GOLD catalog consists of basic astrometry, photometry, and object classification for 25,227,559 objects.
- des_sva1.gold_im3shapeThis catalog includes the shear estimates made using the Im3Shape algorithm, described in Section 7.3 of Jarvis et al, 2015.
- des_sva1.gold_ngmixThis catalog includes the shear estimates made using the NGMix algorithm, described in Section 7.4 of Jarvis et al, 2015.
- des_sva1.gold_skynet_pdfThe PDFs have the following binning in redshift: z_min = 0.005, z_max = 1.8, nbins = 200
- des_sva1.gold_skynet_pointThe structure of the point estimate files are identical. They each contain two columns: the SVA1 unique object identifier and the mean photo-z for that object.
- des_sva1.gold_tpz_pdfThe PDFs have the following binning in redshift: z_min = 0.0012625, z_max = 1.9962625, nbins = 200
- des_sva1.gold_tpz_pointThe structure of the point estimate files are identical. They each contain two columns: the SVA1 unique object identifier and the mean photo-z for that object.
- des_sva1.gold_wlinfoThis catalog is merely for convenience, containing only information derived from other SVA1 catalogs.
- des_sva1.redmagic_brightredMaGiC red galaxy catalog; bright redMaGiC samples. See Rozo et al. (2015), Table B2.
- des_sva1.redmagic_faintredMaGiC red galaxy catalog; faint redMaGiC samples. See Rozo et al. (2015), Table B2.
- des_sva1.redmapper_exp_areaThe RedMaPPer expanded catalog. Effective Area. See Rykoff et al. (2016), Table 12.
- des_sva1.redmapper_exp_catalogThe RedMaPPer expanded catalog. Cluster Catalog. See Rykoff et al. (2016), Table 8.
- des_sva1.redmapper_exp_membersThe RedMaPPer expanded catalog. Member Catalog. See Rykoff et al. (2016), Table 9.
- des_sva1.redmapper_exp_randomsThe RedMaPPer expanded catalog. Random Point. See Rykoff et al. (2016), Table 11.
- des_sva1.redmapper_exp_zmaskThe RedMaPPer expanded catalog. Zmask. See Rykoff et al. (2016), Table 10.
- des_sva1.redmapper_pub_areaThe fiducial catalog with a more conservative footprint and star/galaxy separation. Effective Area. See Rykoff et al. (2016), Table 12.
- des_sva1.redmapper_pub_catalogThe fiducial catalog with a more conservative footprint and star/galaxy separation. Cluster Catalog. See Rykoff et al. (2016), Table 8.
- des_sva1.redmapper_pub_membersThe fiducial catalog with a more conservative footprint and star/galaxy separation. Member Catalog. See Rykoff et al. (2016), Table 9.
- des_sva1.redmapper_pub_randomsThe fiducial catalog with a more conservative footprint and star/galaxy separation. Random Point. See Rykoff et al. (2016), Table 11.
- des_sva1.redmapper_pub_zmaskThe fiducial catalog with a more conservative footprint and star/galaxy separation. Zmask. See Rykoff et al. (2016), Table 10.
- desi_edr
- desi_edr.exposureSummary quantities for every DESI exposure
- desi_edr.fiberassignQuantities obtained when a DESI target is assigned to a fiber
- desi_edr.frameSummary quantities for each petal of the DESI instrument in a given exposure; in normal operation there are ten frames for every exposure
- desi_edr.photometryPhotometric quantities from LS DR9 for every TARGETID
- desi_edr.potentialFor a given tile, this table lists all targets that could have received a fiber assignment
- desi_edr.targetThe quantities obtained when photometric objects are analyzed in the target selection process
- desi_edr.tileSummary quantities for every DESI tile (pointing on the sky)
- desi_edr.x1p5__zpix__allwise__sourcedesi_edr.zpix and xmatch_std.allwise__source crossmatch (1.5 arcsec)
- desi_edr.x1p5__zpix__gaia_dr3__gaia_sourcedesi_edr.zpix and xmatch_std.gaia_dr3__gaia_source crossmatch (1.5 arcsec)
- desi_edr.x1p5__zpix__nsc_dr2__objectdesi_edr.zpix and xmatch_std.nsc_dr2__object crossmatch (1.5 arcsec)
- desi_edr.x1p5__zpix__sdss_dr17__specobjdesi_edr.zpix and xmatch_std.sdss_dr17__specobj crossmatch (1.5 arcsec)
- desi_edr.x1p5__zpix__unwise_dr1__objectdesi_edr.zpix and xmatch_std.unwise_dr1__object crossmatch (1.5 arcsec)
- desi_edr.zpixRedshift and other quantities for spectra that have been grouped and coadded by HEALPixel
- desi_edr.ztileRedshift and other quantities for spectra that have been grouped and coadded by tile
- dltest
- gaia_dr1
- gaia_dr1.cepheidThis table describes the Cepheid stars identified in table VariableSummary as classification=CEP. In the analyses only observations with rejectedByVariabilityProcessing=false are included, as found in table PhotVariableTimeSeriesGfov.
- gaia_dr1.gaia_sourceThis table has an entry for every Gaia observed source as listed in the Main Database accumulating catalogue version from which the catalogue release has been generated. It contains the basic source parameters, that is only final data (no epoch data) and no spectra (neither final nor epoch).
- gaia_dr1.phot_variable_time_series_gfovFOV time series of sources that have phtoVariableFlag=VARIABLE
- gaia_dr1.phot_variable_time_series_gfov_statistical_parametersStatistical parameter of FOV time series
- gaia_dr1.rrlyraeThis table describes the RRLyrae stars identified in table VariableSummary as classification=RRLYR. In the analyses only observations with rejectedByVariabilityProcessing=false are included, as found in table PhotVariableTimeSeriesGfov.
- gaia_dr1.tgas_sourceThis table is a subset of GaiaSource comprising those stars in the Hipparcos and Tycho-2 Catalogues for which a full 5-parameter astrometric solution has been possible in Gaia Data Release 1. This is possible because the early Hipparcos epoch positions break some degeneracies due to the limited Gaia time coverage. This table contains a substantial fraction of the around 2.5 million stars in the Hipparcos and Tycho-2 catalogue. Many stars have been excluded due to several reasons, such as saturation, cross-match errors or bad astrometric solution.
- gaia_dr1.variable_summaryVariability summary of sources with photVariableFlag=VARIABLE
- gaia_dr1.x1p5__gaia_source__allwise__sourcegaia_dr1.gaia_source and allwise.source crossmatch (1.5 arcsec)
- gaia_dr1.x1p5__gaia_source__nsc_dr2__objectgaia_dr1.gaia_source and nsc_dr2.object crossmatch (1.5 arcsec)
- gaia_dr1.x1p5__gaia_source__sdss_dr16__specobjgaia_dr1.gaia_source and sdss_dr16.specobj crossmatch (1.5 arcsec)
- gaia_dr1.x1p5__gaia_source__unwise_dr1__objectgaia_dr1.gaia_source and unwise_dr1.object crossmatch (1.5 arcsec)
- gaia_dr2
- gaia_dr2.cepheidCepheid stars (Gaia collaboration)
- gaia_dr2.gaia_sourcePrimary object table
- gaia_dr2.iersIERS GaiaDR2 cross-identification
- gaia_dr2.light_curvesLight-curve data
- gaia_dr2.lpvLong Period Variable stars (Gaia collaboration)
- gaia_dr2.nsc_dr11.5-arcsec positional crossmatch against NSC DR1
- gaia_dr2.numtransCalibrated FoV transit photometry from CU5, consolidated and provided by CU7 for variable stars in Gaia DR2 (epoch_photometry, part 1) ( Gaia collaboration)
- gaia_dr2.rmRotation period in segment, part 1 (vari_rotation_modulation) (Gaia collaboration)
- gaia_dr2.rmoutRotation period in segment, part 3 (vari_rotation_modulation) (Gaia collaboration)
- gaia_dr2.rmsegRotation period in segment, part 2 (vari_rotation_modulation) (Gaia collaboration)
- gaia_dr2.rrlyraeRR Lyrae stars (vari_rrlyrae) (Gaia collaboration)
- gaia_dr2.rvstdcatMean radial velocities on absolute scale (Gaia collaboration)
- gaia_dr2.rvstdmesOriginal ground-based radial velocity measurements (Gaia collaboration)
- gaia_dr2.shorttsShort-timescale sources (vari_short_timescale) (Gaia collaboration)
- gaia_dr2.ssoobjData related to Solar System objects observed by Gaia (sso_source) (Gaia collaboration)
- gaia_dr2.ssoobsSolar System object observations (sso_observation) (Gaia collaboration)
- gaia_dr2.ssoorbAuxiliary information on asteroid orbits and basic photometric parameters (aux_sso_orbits) (Gaia collaboration)
- gaia_dr2.ssoresResiduals with respect to an orbital fit considering only the Gaia observations (aux_sso_orbit_residuals) (Gaia collaboration)
- gaia_dr2.transitCalibrated FoV transit photometry for CU5, consolidated and provided by CU7 for variable stars in Gaia DR2 (epoch_photometry, part 2) (Gaia collaboration)
- gaia_dr2.tsstatStatistical parameters of time series, using only transits not rejected (vari_time_series_statistics) (Gaia collaboration)
- gaia_dr2.varresVariability classification results of all classifiers, identified by the classifierName column (vari_classifier_result) (Gaia collaboration)
- gaia_dr2.x1p5__gaia_source__allwise__sourcegaia_dr2.gaia_source and allwise.source crossmatch (1.5 arcsec)
- gaia_dr2.x1p5__gaia_source__nsc_dr2__objectgaia_dr2.gaia_source and nsc_dr2.object crossmatch (1.5 arcsec)
- gaia_dr2.x1p5__gaia_source__unwise_dr1__objectgaia_dr2.gaia_source and unwise_dr1.object crossmatch (1.5 arcsec)
- gaia_dr3
- gaia_dr3.astrophysical_parameters1D astrophysical parameters produced by the Apsis processing chain developed in Gaia DPAC CU8
- gaia_dr3.gaia_sourceThis table has an entry for every Gaia observed source as published with this data release. It contains the basic source parameters, in their final state as processed by the Gaia Data Processing and Analysis Consortium from the raw data coming from the spacecraft.
- gaia_dr3.galaxy_candidatesThis table contains parameters derived from various modules dedicated to the classification and characterisation of sources considered as galaxy candidates.
- gaia_dr3.qso_candidatesThis table contains parameters derived from various modules dedicated to the classification and characterisation of sources considered as QSO candidates. Together with those, the QSOs used to define the Gaia-CRF3 are also listed in this table.
- gaia_dr3.x1p5__gaia_source__allwise__sourcegaia_dr3.gaia_source and xmatch_std.allwise__source crossmatch (1.5 arcsec)
- gaia_dr3.x1p5__gaia_source__catwise2020__mainxmatch_std.gaia_dr3__gaia_source and catwise2020.main crossmatch (1.5 arcsec)
- gaia_dr3.x1p5__gaia_source__decaps_dr1__objectgaia_dr3.gaia_source and xmatch_std.decaps_dr1__object crossmatch (1.5 arcsec)
- gaia_dr3.x1p5__gaia_source__decaps_dr2__objectgaia_dr3.gaia_source and decaps_dr2.object crossmatch (1.5 arcsec)
- gaia_dr3.x1p5__gaia_source__delve_dr1__objectsgaia_dr3.gaia_source and delve_dr1.objects crossmatch (1.5 arcsec)
- gaia_dr3.x1p5__gaia_source__delve_dr2__objectsgaia_dr3.gaia_source and delve_dr2.objects crossmatch (1.5 arcsec)
- gaia_dr3.x1p5__gaia_source__des_dr1__maingaia_dr3.gaia_source and des_dr1.main crossmatch (1.5 arcsec)
- gaia_dr3.x1p5__gaia_source__des_dr2__maingaia_dr3.gaia_source and xmatch_std.des_dr2__main crossmatch (1.5 arcsec)
- gaia_dr3.x1p5__gaia_source__desi_edr__zpixxmatch_std.gaia_dr3__gaia_source and desi_edr.zpix crossmatch (1.5 arcsec)
- gaia_dr3.x1p5__gaia_source__gnirs_dqs__spec_measurementsgaia_dr3.gaia_source and gnirs_dqs.spec_measurements crossmatch (1.5 arcsec)
- gaia_dr3.x1p5__gaia_source__gogreen_dr1__photogaia_dr3.gaia_source and gogreen_dr1.photo crossmatch (1.5 arcsec)
- gaia_dr3.x1p5__gaia_source__gogreen_dr1__redshiftgaia_dr3.gaia_source and gogreen_dr1.redshift crossmatch (1.5 arcsec)
- gaia_dr3.x1p5__gaia_source__ls_dr10__tractorxmatch_std.gaia_dr3__gaia_source and ls_dr10.tractor crossmatch (1.5 arcsec)
- gaia_dr3.x1p5__gaia_source__ls_dr8__tractorgaia_dr3.gaia_source and ls_dr8.tractor crossmatch (1.5 arcsec)
- gaia_dr3.x1p5__gaia_source__ls_dr9__tractorgaia_dr3.gaia_source and xmatch_std.ls_dr9__tractor crossmatch (1.5 arcsec)
- gaia_dr3.x1p5__gaia_source__nsc_dr2__objectgaia_dr3.gaia_source and xmatch_std.nsc_dr2__object crossmatch (1.5 arcsec)
- gaia_dr3.x1p5__gaia_source__phat_v2__phot_modgaia_dr3.gaia_source and xmatch_std.phat_v2__phot_mod crossmatch (1.5 arcsec)
- gaia_dr3.x1p5__gaia_source__sdss_dr12__specobjgaia_dr3.gaia_source and sdss_dr12.specobj crossmatch (1.5 arcsec)
- gaia_dr3.x1p5__gaia_source__sdss_dr13__specobjgaia_dr3.gaia_source and sdss_dr13.specobj crossmatch (1.5 arcsec)
- gaia_dr3.x1p5__gaia_source__sdss_dr14__specobjgaia_dr3.gaia_source and sdss_dr14.specobj crossmatch (1.5 arcsec)
- gaia_dr3.x1p5__gaia_source__sdss_dr16__specobjgaia_dr3.gaia_source and xmatch_std.sdss_dr16__specobj crossmatch (1.5 arcsec)
- gaia_dr3.x1p5__gaia_source__sdss_dr17__specobjgaia_dr3.gaia_source and sdss_dr17.specobj crossmatch (1.5 arcsec)
- gaia_dr3.x1p5__gaia_source__sga2020__tractorgaia_dr3.gaia_source and sga2020.tractor crossmatch (1.5 arcsec)
- gaia_dr3.x1p5__gaia_source__skymapper_dr1__mastergaia_dr3.gaia_source and skymapper_dr1.master crossmatch (1.5 arcsec)
- gaia_dr3.x1p5__gaia_source__skymapper_dr2__mastergaia_dr3.gaia_source and xmatch_std.skymapper_dr2__master crossmatch (1.5 arcsec)
- gaia_dr3.x1p5__gaia_source__smash_dr1__objectgaia_dr3.gaia_source and smash_dr1.object crossmatch (1.5 arcsec)
- gaia_dr3.x1p5__gaia_source__smash_dr2__objectgaia_dr3.gaia_source and xmatch_std.smash_dr2__object crossmatch (1.5 arcsec)
- gaia_dr3.x1p5__gaia_source__splus_dr1__stripe82gaia_dr3.gaia_source and splus_dr1.stripe82 crossmatch (1.5 arcsec)
- gaia_dr3.x1p5__gaia_source__splus_dr2__maingaia_dr3.gaia_source and xmatch_std.splus_dr2__main crossmatch (1.5 arcsec)
- gaia_dr3.x1p5__gaia_source__splus_edr__stripe82gaia_dr3.gaia_source and splus_edr.stripe82 crossmatch (1.5 arcsec)
- gaia_dr3.x1p5__gaia_source__twomass__pscgaia_dr3.gaia_source and xmatch_std.twomass__psc crossmatch (1.5 arcsec)
- gaia_dr3.x1p5__gaia_source__twomass__xscgaia_dr3.gaia_source and xmatch_std.twomass__xsc crossmatch (1.5 arcsec)
- gaia_dr3.x1p5__gaia_source__tycho2__maingaia_dr3.gaia_source and tycho2.main crossmatch (1.5 arcsec)
- gaia_dr3.x1p5__gaia_source__ukidss_dr11plus__dxssourcegaia_dr3.gaia_source and ukidss_dr11plus.dxssource crossmatch (1.5 arcsec)
- gaia_dr3.x1p5__gaia_source__ukidss_dr11plus__gcssourcegaia_dr3.gaia_source and ukidss_dr11plus.gcssource crossmatch (1.5 arcsec)
- gaia_dr3.x1p5__gaia_source__ukidss_dr11plus__gpssourcegaia_dr3.gaia_source and ukidss_dr11plus.gpssource crossmatch (1.5 arcsec)
- gaia_dr3.x1p5__gaia_source__ukidss_dr11plus__lassourcegaia_dr3.gaia_source and ukidss_dr11plus.lassource crossmatch (1.5 arcsec)
- gaia_dr3.x1p5__gaia_source__ukidss_dr11plus__udssourcegaia_dr3.gaia_source and ukidss_dr11plus.udssource crossmatch (1.5 arcsec)
- gaia_dr3.x1p5__gaia_source__unwise_dr1__objectgaia_dr3.gaia_source and xmatch_std.unwise_dr1__object crossmatch (1.5 arcsec)
- gaia_dr3.x1p5__gaia_source__usno__a2gaia_dr3.gaia_source and xmatch_std.usno__a2 crossmatch (1.5 arcsec)
- gaia_dr3.x1p5__gaia_source__usno__b1gaia_dr3.gaia_source and xmatch_std.usno__b1 crossmatch (1.5 arcsec)
- gaia_dr3.x1p5__gaia_source__vhs_dr5__vhs_cat_v3gaia_dr3.gaia_source and xmatch_std.vhs_dr5__vhs_cat_v3 crossmatch (1.5 arcsec)
- gaia_edr3
- gaia_edr3.agn_cross_idThis table lists sources whose positions and proper motions define the celestial reference frame of Gaia catalogue.
- gaia_edr3.commanded_scan_lawThis table provides a representation of the Gaia scanning law over the 34 month time period covered by the Gaia Data Release 3 (from 2014-07-25 10:31:26 to 2017-05-28 08:46:29), including the Ecliptic Pole Scanning at the begin of the mission.
- gaia_edr3.frame_rotator_sourceSources used to compute the Gaia reference frame.
- gaia_edr3.gaia_sourceThis table has an entry for every Gaia observed source as listed in the Main Database accumulating catalogue version from which the catalogue release has been generated. It contains the basic source parameters, that is only final data (no epoch data) and no spectra (neither final nor epoch). Documentation: https://gea.esac.esa.int/archive/documentation/GEDR3/Gaia_archive/chap_datamodel/sec_dm_main_tables/ssec_dm_gaia_source.html
- gnirs_dqs
- gnirs_dqs.gaussian_fit_parametersGaussian parameters of emission-line profiles
- gnirs_dqs.obs_logObservation log
- gnirs_dqs.spec_measurementsSpectral measurements
- gnirs_dqs.spec_measurements_suppSupplementary spectral measurements
- gnirs_dqs.x1p5__spec_measurements__allwise__sourcegnirs_dqs.spec_measurements and xmatch_std.allwise__source crossmatch (1.5 arcsec)
- gnirs_dqs.x1p5__spec_measurements__gaia_dr3__gaia_sourcegnirs_dqs.spec_measurements and gaia_dr3.gaia_source crossmatch (1.5 arcsec)
- gnirs_dqs.x1p5__spec_measurements__nsc_dr2__objectgnirs_dqs.spec_measurements and xmatch_std.nsc_dr2__object crossmatch (1.5 arcsec)
- gnirs_dqs.x1p5__spec_measurements__sdss_dr17__specobjgnirs_dqs.spec_measurements and sdss_dr17.specobj crossmatch (1.5 arcsec)
- gnirs_dqs.x1p5__spec_measurements__unwise_dr1__objectgnirs_dqs.spec_measurements and xmatch_std.unwise_dr1__object crossmatch (1.5 arcsec)
- gogreen_dr1
- gogreen_dr1.clustersinformation relevant to each cluster in system in the GCLASS and GOGREEN surveys
- gogreen_dr1.photoselected photometric data for each cluster system in the GCLASS, GOGREEN samples, COMOS UltraVISTA, and SXDF SPLASH fields
- gogreen_dr1.redshiftcontains an entry for every unique object with a GOGREEN or GCLASS spectrum
- gogreen_dr1.x1p5__photo__allwise__sourcegogreen_dr1.photo and allwise.source crossmatch (1.5 arcsec)
- gogreen_dr1.x1p5__photo__gaia_dr3__gaia_sourcegogreen_dr1.photo and gaia_dr3.gaia_source crossmatch (1.5 arcsec)
- gogreen_dr1.x1p5__photo__nsc_dr2__objectgogreen_dr1.photo and nsc_dr2.object crossmatch (1.5 arcsec)
- gogreen_dr1.x1p5__photo__sdss_dr17__specobjgogreen_dr1.photo and sdss_dr17.specobj crossmatch (1.5 arcsec)
- gogreen_dr1.x1p5__photo__unwise_dr1__objectgogreen_dr1.photo and unwise_dr1.object crossmatch (1.5 arcsec)
- gogreen_dr1.x1p5__redshift__allwise__sourcegogreen_dr1.redshift and allwise.source crossmatch (1.5 arcsec)
- gogreen_dr1.x1p5__redshift__gaia_dr3__gaia_sourcegogreen_dr1.redshift and gaia_dr3.gaia_source crossmatch (1.5 arcsec)
- gogreen_dr1.x1p5__redshift__nsc_dr2__objectgogreen_dr1.redshift and nsc_dr2.object crossmatch (1.5 arcsec)
- gogreen_dr1.x1p5__redshift__sdss_dr17__specobjgogreen_dr1.redshift and sdss_dr17.specobj crossmatch (1.5 arcsec)
- gogreen_dr1.x1p5__redshift__unwise_dr1__objectgogreen_dr1.redshift and unwise_dr1.object crossmatch (1.5 arcsec)
- hipparcos
- hipparcos2
- ls_dr10
- ls_dr10.apfluxAperture flux values of tractor objects (combined DR10 southern region and DR9 northern region)
- ls_dr10.apflux_sAperture flux values of tractor objects (DR10 southern region)
- ls_dr10.bricksTable with RA, Dec bounds of each geometrical brick on the sky
- ls_dr10.bricks_sTable with RA, Dec bounds of each geometrical brick on the sky (DR10 southern region)
- ls_dr10.depth_summary_sA concatenation of the depth histograms for each brick (DR10 southern region)
- ls_dr10.tractorMain tractor photometry catalog (combined DR10 southern region and DR9 northern region); Less frequently used columns placed in apflux and wise tables
- ls_dr10.tractor_sMain tractor photometry catalog (DR10 southern region); Less frequently used columns placed in apflux and wise tables
- ls_dr10.wiseWISE photometry of objects in combined DR10 southern region and DR9 northern region
- ls_dr10.wise_sWISE photometry of objects in DR10 southern region
- ls_dr10.x1p5__tractor__allwise__sourcels_dr10.tractor and xmatch_std.allwise__source crossmatch (1.5 arcsec)
- ls_dr10.x1p5__tractor__gaia_dr3__gaia_sourcels_dr10.tractor and xmatch_std.gaia_dr3__gaia_source crossmatch (1.5 arcsec)
- ls_dr10.x1p5__tractor__nsc_dr2__objectls_dr10.tractor and xmatch_std.nsc_dr2__object crossmatch (1.5 arcsec)
- ls_dr10.x1p5__tractor__sdss_dr17__specobjls_dr10.tractor and xmatch_std.sdss_dr17__specobj crossmatch (1.5 arcsec)
- ls_dr10.x1p5__tractor__unwise_dr1__objectls_dr10.tractor and xmatch_std.unwise_dr1__object crossmatch (1.5 arcsec)
- ls_dr8
- ls_dr8.apfluxAperture flux values of tractor objects combined regions
- ls_dr8.apflux_nAperture flux values of tractor objects (northern region)
- ls_dr8.apflux_sAperture flux values of tractor objects (southern region)
- ls_dr8.bricksTable with RA, Dec bounds of each geometrical brick on the entire sky (survey-bricks)
- ls_dr8.bricks_nTable with RA, DEC bounds of each geometrical brick on the sky (northern region)
- ls_dr8.bricks_sTable with RA, DEC bounds of each geometrical brick on the sky (southern region)
- ls_dr8.ccds_annotatedAdditional information gathered during calibration pre-processing before running the Tractor reductions.
- ls_dr8.depth_nA concatenation of the depth histograms for each brick (northern region)
- ls_dr8.depth_sA concatenation of the depth histograms for each brick (southern region)
- ls_dr8.depth_summary_nA summary of the depth histogram of the whole dr8 survey (northern region)
- ls_dr8.depth_summary_sA summary of the depth histogram of the whole dr8 survey (southern region)
- ls_dr8.dr8_north_dr12qSDSS DR12 QSO crossmatch
- ls_dr8.dr8_north_dr14q_v4_4SDSS DR14_v4.4 QSO crossmatch
- ls_dr8.dr8_north_dr7qSDSS DR7 QSO crossmatch
- ls_dr8.dr8_north_specobj_dr14SDSS DR14 spectra
- ls_dr8.dr8_north_superset_dr12qSDSS DR12 QSO Superset
- ls_dr8.dr8_south_dr12qSDSS DR12 QSO crossmatch
- ls_dr8.dr8_south_dr14q_v4_4SDSS DR14_v4.4 QSO crossmatch
- ls_dr8.dr8_south_dr7qSDSS DR7 QSO crossmatch
- ls_dr8.dr8_south_specobj_dr14SDSS DR14 spectra
- ls_dr8.dr8_south_superset_dr12qSDSS DR12 QSO Superset
- ls_dr8.forcedForced photometry results, for all CCDs that were included in the DR8 processing.
- ls_dr8.photo_zPhotometric redshift
- ls_dr8.survey_ccds_kd_nA table with almanac information (e.g. seeing, etc.) about each individual CCD image limited by depth (northern region)
- ls_dr8.survey_ccds_kd_sA table with almanac information (e.g. seeing, etc.) about each individual CCD image limited by depth (southern region)
- ls_dr8.tractorMain tractor photometry catalog (combined north and south regions); Less frequently used columns placed in apflux and wise tables
- ls_dr8.tractor_nMain tractor photometry catalog (northern region); Less frequently used columns placed in apflux_s and wise_s tables
- ls_dr8.tractor_sMain tractor photometry catalog (southern region); Less frequently used columns placed in apflux_s and wise_s tables
- ls_dr8.wiseWISE photometry of objects combined regions
- ls_dr8.wise_nWISE photometry of objects (northern region)
- ls_dr8.wise_sWISE photometry of objects (southern region)
- ls_dr8.x1p5__tractor__allwise__sourcels_dr8.tractor and xmatch_std.allwise__source crossmatch (1.5 arcsec)
- ls_dr8.x1p5__tractor__gaia_dr3__gaia_sourcels_dr8.tractor and gaia_dr3.gaia_source crossmatch (1.5 arcsec)
- ls_dr8.x1p5__tractor__nsc_dr2__objectls_dr8.tractor and xmatch_std.nsc_dr2__object crossmatch (1.5 arcsec)
- ls_dr8.x1p5__tractor__sdss_dr17__specobjls_dr8.tractor and sdss_dr17.specobj crossmatch (1.5 arcsec)
- ls_dr8.x1p5__tractor__unwise_dr1__objectls_dr8.tractor and xmatch_std.unwise_dr1__object crossmatch (1.5 arcsec)
- ls_dr9
- ls_dr9.apfluxAperture flux values of tractor objects
- ls_dr9.apflux_nAperture flux values of tractor objects (northern region)
- ls_dr9.apflux_sAperture flux values of tractor objects (southern region)
- ls_dr9.bricksTable with RA, Dec bounds of each geometrical brick on the entire sky (survey-bricks)
- ls_dr9.bricks_nTable with RA, DEC bounds of each geometrical brick on the sky (Northern region)
- ls_dr9.bricks_sTable with RA, DEC bounds of each geometrical brick on the sky (Southern region)
- ls_dr9.ccds_annotatedAdditional information gathered during calibration pre-processing before running the Tractor reductions
- ls_dr9.depth_summary_nA concatenation of the depth histograms for each brick (Northern region)
- ls_dr9.depth_summary_sA concatenation of the depth histograms for each brick (Southern region)
- ls_dr9.forcedForced photometry results, for all CCDs that were included in the DR9 processing
- ls_dr9.photo_zPhotometric redshift
- ls_dr9.tractorMain tractor photometry catalog (combined north and south regions); Less frequently used columns placed in apflux and wise tables
- ls_dr9.tractor_nMain tractor photometry catalog (north region); Less frequently used columns placed in apflux and wise tables
- ls_dr9.tractor_sMain tractor photometry catalog (south region); Less frequently used columns placed in apflux and wise tables
- ls_dr9.wiseWISE photometry of objects in combined region
- ls_dr9.wise_nWISE photometry of objects in northern region
- ls_dr9.wise_sWISE photometry of objects in southern region
- ls_dr9.x1p5__tractor__allwise__sourcexmatch_std.ls_dr9__tractor and xmatch_std.allwise__source crossmatch (1.5 arcsec)
- ls_dr9.x1p5__tractor__gaia_dr3__gaia_sourcexmatch_std.ls_dr9__tractor and gaia_dr3.gaia_source crossmatch (1.5 arcsec)
- ls_dr9.x1p5__tractor__nsc_dr2__objectxmatch_std.ls_dr9__tractor and xmatch_std.nsc_dr2__object crossmatch (1.5 arcsec)
- ls_dr9.x1p5__tractor__sdss_dr17__specobjxmatch_std.ls_dr9__tractor and sdss_dr17.specobj crossmatch (1.5 arcsec)
- ls_dr9.x1p5__tractor__unwise_dr1__objectxmatch_std.ls_dr9__tractor and xmatch_std.unwise_dr1__object crossmatch (1.5 arcsec)
- ls_dr9sv
- ls_dr9sv.apflux_nAperture flux values of tractor objects (northern region)
- ls_dr9sv.apflux_sAperture flux values of tractor objects (southern region)
- ls_dr9sv.tractor_nMain tractor photometry catalog (northern region): Less frequently used columns placed in apflux_n and wise_n tables
- ls_dr9sv.tractor_primary_nPrimary-object tractor photometry catalog
- ls_dr9sv.tractor_primary_sPrimary-object tractor photometry catalog
- ls_dr9sv.tractor_sMain tractor photometry catalog (southern region): Less frequently used columns placed in apflux_s and wise_s tables
- ls_dr9sv.tractor_secondary_nSecondary-object tractor photometry catalog
- ls_dr9sv.tractor_secondary_sSecondary-object tractor photometry catalog
- ls_dr9sv.wise_nWISE photometry of objects (northern region)
- ls_dr9sv.wise_sWISE photometry of objects (southern region)
- lsst_sim
- nsc_dr1
- nsc_dr1.chipCCD information table
- nsc_dr1.coverageSurvey coverage table
- nsc_dr1.exposureExposures contributing to the catalog
- nsc_dr1.measPrimary measurements table
- nsc_dr1.nsc_allwiseNSC vs ALLWISE 1-arcsec crossmatch
- nsc_dr1.objectPrimary object table
- nsc_dr1.x1p5__object__decaps_dr1__objectnsc_dr1.object and decaps_dr1.object crossmatch (1.5 arcsec)
- nsc_dr1.x1p5__object__des_dr1__mainnsc_dr1.object and des_dr1.main crossmatch (1.5 arcsec)
- nsc_dr1.x1p5__object__gaia_dr1__gaia_sourcensc_dr1.object and gaia_dr1.gaia_source crossmatch (1.5 arcsec)
- nsc_dr1.x1p5__object__gaia_dr2__gaia_sourcensc_dr1.object and gaia_dr2.gaia_source crossmatch (1.5 arcsec)
- nsc_dr1.x1p5__object__gogreen_dr1__photonsc_dr1.object and gogreen_dr1.photo crossmatch (1.5 arcsec)
- nsc_dr1.x1p5__object__gogreen_dr1__redshiftnsc_dr1.object and gogreen_dr1.redshift crossmatch (1.5 arcsec)
- nsc_dr1.x1p5__object__sdss_dr12__specobjnsc_dr1.object and sdss_dr12.specobj crossmatch (1.5 arcsec)
- nsc_dr1.x1p5__object__sdss_dr13__specobjnsc_dr1.object and sdss_dr13.specobj crossmatch (1.5 arcsec)
- nsc_dr1.x1p5__object__sdss_dr14__specobjnsc_dr1.object and sdss_dr14.specobj crossmatch (1.5 arcsec)
- nsc_dr1.x1p5__object__sdss_dr16__specobjnsc_dr1.object and sdss_dr16.specobj crossmatch (1.5 arcsec)
- nsc_dr1.x1p5__object__smash_dr1__objectnsc_dr1.object and smash_dr1.object crossmatch (1.5 arcsec)
- nsc_dr1.x1p5__object__smash_dr2__objectnsc_dr1.object and smash_dr2.object crossmatch (1.5 arcsec)
- nsc_dr1.x1p5__object__splus_dr1__stripe82nsc_dr1.object and splus_dr1.stripe82 crossmatch (1.5 arcsec)
- nsc_dr1.x1p5__object__splus_edr__stripe82nsc_dr1.object and splus_edr.stripe82 crossmatch (1.5 arcsec)
- nsc_dr1.x1p5__object__twomass__xscnsc_dr1.object and twomass.xsc crossmatch (1.5 arcsec)
- nsc_dr1.x1p5__object__tycho2__mainnsc_dr1.object and tycho2.main crossmatch (1.5 arcsec)
- nsc_dr1.x1p5__object__unwise_dr1__objectnsc_dr1.object and unwise_dr1.object crossmatch (1.5 arcsec)
- nsc_dr1.x1p5__object__usno__a2nsc_dr1.object and usno.a2 crossmatch (1.5 arcsec)
- nsc_dr1.x1p5__object__usno__b1nsc_dr1.object and usno.b1 crossmatch (1.5 arcsec)
- nsc_dr2
- nsc_dr2.chipCCD information table
- nsc_dr2.coverageSurvey coverage table
- nsc_dr2.exposureExposures contributing to the catalog
- nsc_dr2.measPrimary measurements table
- nsc_dr2.objectPrimary object table
- nsc_dr2.x1p5__object__allwise__sourcensc_dr2.object and allwise.source crossmatch (1.5 arcsec)
- nsc_dr2.x1p5__object__catwise2020__mainxmatch_std.nsc_dr2__object and catwise2020.main crossmatch (1.5 arcsec)
- nsc_dr2.x1p5__object__decaps_dr1__objectnsc_dr2.object and decaps_dr1.object crossmatch (1.5 arcsec)
- nsc_dr2.x1p5__object__decaps_dr2__objectxmatch_std.nsc_dr2__object and decaps_dr2.object crossmatch (1.5 arcsec)
- nsc_dr2.x1p5__object__delve_dr1__objectsnsc_dr2.object and delve_dr1.objects crossmatch (1.5 arcsec)
- nsc_dr2.x1p5__object__delve_dr2__objectsxmatch_std.nsc_dr2__object and delve_dr2.objects crossmatch (1.5 arcsec)
- nsc_dr2.x1p5__object__des_dr1__mainnsc_dr2.object and des_dr1.main crossmatch (1.5 arcsec)
- nsc_dr2.x1p5__object__des_dr2__mainnsc_dr2.object and des_dr2.main crossmatch (1.5 arcsec)
- nsc_dr2.x1p5__object__desi_edr__zpixxmatch_std.nsc_dr2__object and desi_edr.zpix crossmatch (1.5 arcsec)
- nsc_dr2.x1p5__object__gaia_dr1__gaia_sourcensc_dr2.object and gaia_dr1.gaia_source crossmatch (1.5 arcsec)
- nsc_dr2.x1p5__object__gaia_dr2__gaia_sourcensc_dr2.object and gaia_dr2.gaia_source crossmatch (1.5 arcsec)
- nsc_dr2.x1p5__object__gaia_dr3__gaia_sourcexmatch_std.nsc_dr2__object and gaia_dr3.gaia_source crossmatch (1.5 arcsec)
- nsc_dr2.x1p5__object__gnirs_dqs__spec_measurementsxmatch_std.nsc_dr2__object and gnirs_dqs.spec_measurements crossmatch (1.5 arcsec)
- nsc_dr2.x1p5__object__gogreen_dr1__photonsc_dr2.object and gogreen_dr1.photo crossmatch (1.5 arcsec)
- nsc_dr2.x1p5__object__gogreen_dr1__redshiftnsc_dr2.object and gogreen_dr1.redshift crossmatch (1.5 arcsec)
- nsc_dr2.x1p5__object__ls_dr10__tractorxmatch_std.nsc_dr2__object and ls_dr10.tractor crossmatch (1.5 arcsec)
- nsc_dr2.x1p5__object__ls_dr8__tractorxmatch_std.nsc_dr2__object and ls_dr8.tractor crossmatch (1.5 arcsec)
- nsc_dr2.x1p5__object__ls_dr9__tractorxmatch_std.nsc_dr2__object and xmatch_std.ls_dr9__tractor crossmatch (1.5 arcsec)
- nsc_dr2.x1p5__object__sdss_dr12__specobjnsc_dr2.object and sdss_dr12.specobj crossmatch (1.5 arcsec)
- nsc_dr2.x1p5__object__sdss_dr13__specobjnsc_dr2.object and sdss_dr13.specobj crossmatch (1.5 arcsec)
- nsc_dr2.x1p5__object__sdss_dr14__specobjnsc_dr2.object and sdss_dr14.specobj crossmatch (1.5 arcsec)
- nsc_dr2.x1p5__object__sdss_dr16__specobjnsc_dr2.object and sdss_dr16.specobj crossmatch (1.5 arcsec)
- nsc_dr2.x1p5__object__sdss_dr17__specobjxmatch_std.nsc_dr2__object and sdss_dr17.specobj crossmatch (1.5 arcsec)
- nsc_dr2.x1p5__object__sga2020__tractorxmatch_std.nsc_dr2__object and sga2020.tractor crossmatch (1.5 arcsec)
- nsc_dr2.x1p5__object__skymapper_dr1__masternsc_dr2.object and skymapper_dr1.master crossmatch (1.5 arcsec)
- nsc_dr2.x1p5__object__skymapper_dr2__masterxmatch_std.nsc_dr2__object and skymapper_dr2.master crossmatch (1.5 arcsec)
- nsc_dr2.x1p5__object__smash_dr1__objectnsc_dr2.object and smash_dr1.object crossmatch (1.5 arcsec)
- nsc_dr2.x1p5__object__smash_dr2__objectnsc_dr2.object and smash_dr2.object crossmatch (1.5 arcsec)
- nsc_dr2.x1p5__object__splus_dr1__stripe82nsc_dr2.object and splus_dr1.stripe82 crossmatch (1.5 arcsec)
- nsc_dr2.x1p5__object__splus_dr2__mainxmatch_std.nsc_dr2__object and splus_dr2.main crossmatch (1.5 arcsec)
- nsc_dr2.x1p5__object__splus_edr__stripe82nsc_dr2.object and splus_edr.stripe82 crossmatch (1.5 arcsec)
- nsc_dr2.x1p5__object__twomass__pscnsc_dr2.object and twomass.psc crossmatch (1.5 arcsec)
- nsc_dr2.x1p5__object__twomass__xscnsc_dr2.object and twomass.xsc crossmatch (1.5 arcsec)
- nsc_dr2.x1p5__object__ukidss_dr11plus__dxssourcexmatch_std.nsc_dr2__object and ukidss_dr11plus.dxssource crossmatch (1.5 arcsec)
- nsc_dr2.x1p5__object__ukidss_dr11plus__gcssourcexmatch_std.nsc_dr2__object and ukidss_dr11plus.gcssource crossmatch (1.5 arcsec)
- nsc_dr2.x1p5__object__ukidss_dr11plus__gpssourcexmatch_std.nsc_dr2__object and ukidss_dr11plus.gpssource crossmatch (1.5 arcsec)
- nsc_dr2.x1p5__object__ukidss_dr11plus__lassourcexmatch_std.nsc_dr2__object and ukidss_dr11plus.lassource crossmatch (1.5 arcsec)
- nsc_dr2.x1p5__object__ukidss_dr11plus__udssourcexmatch_std.nsc_dr2__object and ukidss_dr11plus.udssource crossmatch (1.5 arcsec)
- nsc_dr2.x1p5__object__unwise_dr1__objectnsc_dr2.object and unwise_dr1.object crossmatch (1.5 arcsec)
- nsc_dr2.x1p5__object__usno__a2nsc_dr2.object and usno.a2 crossmatch (1.5 arcsec)
- nsc_dr2.x1p5__object__usno__b1nsc_dr2.object and usno.b1 crossmatch (1.5 arcsec)
- nsc_dr2.x1p5__object__vhs_dr5__vhs_cat_v3nsc_dr2.object and vhs_dr5.vhs_cat_v3 crossmatch (1.5 arcsec)
- phat_v2
- phat_v2.phot_measIndividual photometric measurements, one row per measurement
- phat_v2.phot_modCombined average photometry
- phat_v2.phot_v2Individual photometric measurements in original table format
- phat_v2.star_v2Combined average photometry in original table format
- phat_v2.x1p5__phot_mod__allwise__sourcephat_v2.phot_mod and allwise.source crossmatch (1.5 arcsec)
- phat_v2.x1p5__phot_mod__gaia_dr3__gaia_sourcexmatch_std.phat_v2__phot_mod and gaia_dr3.gaia_source crossmatch (1.5 arcsec)
- phat_v2.x1p5__phot_mod__unwise_dr1__objectphat_v2.phot_mod and unwise_dr1.object crossmatch (1.5 arcsec)
- sdss_dr12
- sdss_dr12.dr12qThe DR12 QSO Catalog.
- sdss_dr12.dr12q_duplicatesA join table linking the spectra in dr12q to other observations of the same object.
- sdss_dr12.emissionlinesportEmission line kinematics results for SDSS and BOSS galaxies using GANDALF
- sdss_dr12.photoplateThe full photometric catalog quantities for SDSS imaging.
- sdss_dr12.platexContains data from a given plate used for spectroscopic observations.
- sdss_dr12.segue1specobjallA view of specobjall that includes only SEGUE-1 spectra.
- sdss_dr12.segue2specobjallA view of specobjall that includes only SEGUE-2 spectra.
- sdss_dr12.seguespecobjallA view of specobjall that includes only SEGUE-1+SEGUE-2 spectra.
- sdss_dr12.specobjA subset of specobjall that just has the clean spectra. The subset excludes QA and Sky and duplicates. Use this as the main way to access the spectro objects.
- sdss_dr12.specobjallContains the measured parameters for a spectrum.
- sdss_dr12.x1p5__specobj__allwise__sourcesdss_dr12.specobj and allwise.source crossmatch (1.5 arcsec)
- sdss_dr12.x1p5__specobj__gaia_dr3__gaia_sourcesdss_dr12.specobj and gaia_dr3.gaia_source crossmatch (1.5 arcsec)
- sdss_dr12.x1p5__specobj__nsc_dr2__objectsdss_dr12.specobj and nsc_dr2.object crossmatch (1.5 arcsec)
- sdss_dr12.x1p5__specobj__sdss_dr17__specobjsdss_dr12.specobj and sdss_dr17.specobj crossmatch (1.5 arcsec)
- sdss_dr12.x1p5__specobj__unwise_dr1__objectsdss_dr12.specobj and unwise_dr1.object crossmatch (1.5 arcsec)
- sdss_dr13
- sdss_dr13.calibobj_galSweep of photObj -- galaxies
- sdss_dr13.calibobj_starSweep of photObj -- stars
- sdss_dr13.dr12qsoDR12 QSO Catalog
- sdss_dr13.emissionlinesport_dr12Emission line kinematics results for SDSS DR12 and BOSS galaxies using GANDALF
- sdss_dr13.galspecline_dr8Emission line measurements from MPA-JHU spectroscopic reanalysis
- sdss_dr13.photoposplatePhotometry of DR13 spectral objects
- sdss_dr13.specobjDR13 SpecObj catalog
- sdss_dr13.wisematch_galSweep of photObj -- galaxies
- sdss_dr13.wisematch_starSweep of photObj -- stars
- sdss_dr13.x1p5__specobj__allwise__sourcesdss_dr13.specobj and allwise.source crossmatch (1.5 arcsec)
- sdss_dr13.x1p5__specobj__gaia_dr3__gaia_sourcesdss_dr13.specobj and gaia_dr3.gaia_source crossmatch (1.5 arcsec)
- sdss_dr13.x1p5__specobj__nsc_dr2__objectsdss_dr13.specobj and nsc_dr2.object crossmatch (1.5 arcsec)
- sdss_dr13.x1p5__specobj__sdss_dr17__specobjsdss_dr13.specobj and sdss_dr17.specobj crossmatch (1.5 arcsec)
- sdss_dr13.x1p5__specobj__unwise_dr1__objectsdss_dr13.specobj and unwise_dr1.object crossmatch (1.5 arcsec)
- sdss_dr14
- sdss_dr14.dr14qThe DR14 QSO Catalog (v4_4, final).
- sdss_dr14.dr14q_duplicatesA join table linking the spectra in dr14q to other observations of the same object.
- sdss_dr14.photoplateThe full photometric catalog quantities for SDSS imaging.
- sdss_dr14.platexContains data from a given plate used for spectroscopic observations.
- sdss_dr14.sdssebossfireflyContains the measured stellar population parameters for a spectrum.
- sdss_dr14.segue1specobjallA view of specobjall that includes only SEGUE-1 spectra.
- sdss_dr14.segue2specobjallA view of specobjall that includes only SEGUE-2 spectra.
- sdss_dr14.seguespecobjallA view of specobjall that includes only SEGUE-1+SEGUE-2 spectra.
- sdss_dr14.specobjA subset of specobjall that just has the clean spectra. The subset excludes QA and Sky and duplicates. Use this as the main way to access the spectro objects.
- sdss_dr14.specobjallContains the measured parameters for a spectrum.
- sdss_dr14.spiders_quasarThe SPIDERS quasar eRosita source
- sdss_dr14.x1p5__specobj__allwise__sourcesdss_dr14.specobj and allwise.source crossmatch (1.5 arcsec)
- sdss_dr14.x1p5__specobj__gaia_dr3__gaia_sourcesdss_dr14.specobj and gaia_dr3.gaia_source crossmatch (1.5 arcsec)
- sdss_dr14.x1p5__specobj__nsc_dr2__objectsdss_dr14.specobj and nsc_dr2.object crossmatch (1.5 arcsec)
- sdss_dr14.x1p5__specobj__sdss_dr17__specobjsdss_dr14.specobj and sdss_dr17.specobj crossmatch (1.5 arcsec)
- sdss_dr14.x1p5__specobj__unwise_dr1__objectsdss_dr14.specobj and unwise_dr1.object crossmatch (1.5 arcsec)
- sdss_dr16
- sdss_dr16.dr16qThe DR16 QSO Catalog (v3)
- sdss_dr16.dr16q_duplicatesThe DR16 QSO Duplicates Catalog (v3)
- sdss_dr16.dr16q_supersetThe DR16 QSO Superset Catalog (v3)
- sdss_dr16.dr16q_superset_duplicatesThe DR16 QSO Superset Duplicates Catalog (v3)
- sdss_dr16.elg_classifierThe DR16 ELG Classifier
- sdss_dr16.photoplateThe full photometric catalog quantities for SDSS imaging.
- sdss_dr16.platexContains data from a given plate used for spectroscopic observations.
- sdss_dr16.sdssebossfireflyContains the measured stellar population parameters for a spectrum.
- sdss_dr16.segue1specobjallA view of specobjall that includes only SEGUE-1 spectra.
- sdss_dr16.segue2specobjallA view of specobjall that includes only SEGUE-2 spectra.
- sdss_dr16.seguespecobjallA view of specobjall that includes only SEGUE-1+SEGUE-2 spectra.
- sdss_dr16.specobjA subset of specobjall that just has the clean spectra. The subset excludes QA and Sky and duplicates. Use this as the main way to access the spectro objects.
- sdss_dr16.specobjallContains the measured parameters for a spectrum.
- sdss_dr16.spiders_quasarThe DR16 SPIDERS quasar eRosita source
- sdss_dr16.x1p5__specobj__allwise__sourcesdss_dr16.specobj and allwise.source crossmatch (1.5 arcsec)
- sdss_dr16.x1p5__specobj__gaia_dr1__gaia_sourcesdss_dr16.specobj and gaia_dr1.gaia_source crossmatch (1.5 arcsec)
- sdss_dr16.x1p5__specobj__gaia_dr3__gaia_sourcexmatch_std.sdss_dr16__specobj and gaia_dr3.gaia_source crossmatch (1.5 arcsec)
- sdss_dr16.x1p5__specobj__nsc_dr2__objectsdss_dr16.specobj and nsc_dr2.object crossmatch (1.5 arcsec)
- sdss_dr16.x1p5__specobj__sdss_dr17__specobjxmatch_std.sdss_dr16__specobj and sdss_dr17.specobj crossmatch (1.5 arcsec)
- sdss_dr16.x1p5__specobj__skymapper_dr1__masterxmatch_std.sdss_dr16__specobj and skymapper_dr1.master crossmatch (1.5 arcsec)
- sdss_dr16.x1p5__specobj__splus_dr1__stripe82sdss_dr16.specobj and splus_dr1.stripe82 crossmatch (1.5 arcsec)
- sdss_dr16.x1p5__specobj__unwise_dr1__objectsdss_dr16.specobj and unwise_dr1.object crossmatch (1.5 arcsec)
- sdss_dr17
- sdss_dr17.photoplateThe full photometric catalog quantities for SDSS imaging.
- sdss_dr17.platexContains data from a given plate used for spectroscopic observations.
- sdss_dr17.segue1specobjallA view of specobjall that includes only SEGUE-1 spectra.
- sdss_dr17.segue2specobjallA view of specobjall that includes only SEGUE-2 spectra.
- sdss_dr17.seguespecobjallA view of specobjall that includes only SEGUE-1+SEGUE-2 spectra.
- sdss_dr17.specobjA view of specobjall that just has the clean spectra. The view excludes QA and Sky and duplicates. Use this as the main way to access the spectro objects.
- sdss_dr17.specobjallContains the measured parameters for a spectrum.
- sdss_dr17.x1p5__specobj__allwise__sourcesdss_dr17.specobj and xmatch_std.allwise__source crossmatch (1.5 arcsec)
- sdss_dr17.x1p5__specobj__catwise2020__mainxmatch_std.sdss_dr17__specobj and catwise2020.main crossmatch (1.5 arcsec)
- sdss_dr17.x1p5__specobj__decaps_dr1__objectsdss_dr17.specobj and xmatch_std.decaps_dr1__object crossmatch (1.5 arcsec)
- sdss_dr17.x1p5__specobj__decaps_dr2__objectsdss_dr17.specobj and decaps_dr2.object crossmatch (1.5 arcsec)
- sdss_dr17.x1p5__specobj__delve_dr1__objectssdss_dr17.specobj and delve_dr1.objects crossmatch (1.5 arcsec)
- sdss_dr17.x1p5__specobj__delve_dr2__objectssdss_dr17.specobj and delve_dr2.objects crossmatch (1.5 arcsec)
- sdss_dr17.x1p5__specobj__des_dr1__mainsdss_dr17.specobj and des_dr1.main crossmatch (1.5 arcsec)
- sdss_dr17.x1p5__specobj__des_dr2__mainsdss_dr17.specobj and xmatch_std.des_dr2__main crossmatch (1.5 arcsec)
- sdss_dr17.x1p5__specobj__desi_edr__zpixxmatch_std.sdss_dr17__specobj and desi_edr.zpix crossmatch (1.5 arcsec)
- sdss_dr17.x1p5__specobj__gaia_dr3__gaia_sourcesdss_dr17.specobj and gaia_dr3.gaia_source crossmatch (1.5 arcsec)
- sdss_dr17.x1p5__specobj__gnirs_dqs__spec_measurementssdss_dr17.specobj and gnirs_dqs.spec_measurements crossmatch (1.5 arcsec)
- sdss_dr17.x1p5__specobj__gogreen_dr1__photosdss_dr17.specobj and gogreen_dr1.photo crossmatch (1.5 arcsec)
- sdss_dr17.x1p5__specobj__gogreen_dr1__redshiftsdss_dr17.specobj and gogreen_dr1.redshift crossmatch (1.5 arcsec)
- sdss_dr17.x1p5__specobj__ls_dr10__tractorxmatch_std.sdss_dr17__specobj and ls_dr10.tractor crossmatch (1.5 arcsec)
- sdss_dr17.x1p5__specobj__ls_dr8__tractorsdss_dr17.specobj and ls_dr8.tractor crossmatch (1.5 arcsec)
- sdss_dr17.x1p5__specobj__ls_dr9__tractorsdss_dr17.specobj and xmatch_std.ls_dr9__tractor crossmatch (1.5 arcsec)
- sdss_dr17.x1p5__specobj__nsc_dr2__objectsdss_dr17.specobj and xmatch_std.nsc_dr2__object crossmatch (1.5 arcsec)
- sdss_dr17.x1p5__specobj__sdss_dr12__specobjsdss_dr17.specobj and sdss_dr12.specobj crossmatch (1.5 arcsec)
- sdss_dr17.x1p5__specobj__sdss_dr13__specobjsdss_dr17.specobj and sdss_dr13.specobj crossmatch (1.5 arcsec)
- sdss_dr17.x1p5__specobj__sdss_dr14__specobjsdss_dr17.specobj and sdss_dr14.specobj crossmatch (1.5 arcsec)
- sdss_dr17.x1p5__specobj__sdss_dr16__specobjsdss_dr17.specobj and xmatch_std.sdss_dr16__specobj crossmatch (1.5 arcsec)
- sdss_dr17.x1p5__specobj__sga2020__tractorsdss_dr17.specobj and sga2020.tractor crossmatch (1.5 arcsec)
- sdss_dr17.x1p5__specobj__skymapper_dr2__mastersdss_dr17.specobj and xmatch_std.skymapper_dr2__master crossmatch (1.5 arcsec)
- sdss_dr17.x1p5__specobj__splus_dr2__mainsdss_dr17.specobj and xmatch_std.splus_dr2__main crossmatch (1.5 arcsec)
- sdss_dr17.x1p5__specobj__splus_edr__stripe82sdss_dr17.specobj and splus_edr.stripe82 crossmatch (1.5 arcsec)
- sdss_dr17.x1p5__specobj__twomass__pscsdss_dr17.specobj and xmatch_std.twomass__psc crossmatch (1.5 arcsec)
- sdss_dr17.x1p5__specobj__twomass__xscsdss_dr17.specobj and xmatch_std.twomass__xsc crossmatch (1.5 arcsec)
- sdss_dr17.x1p5__specobj__tycho2__mainsdss_dr17.specobj and tycho2.main crossmatch (1.5 arcsec)
- sdss_dr17.x1p5__specobj__ukidss_dr11plus__dxssourcesdss_dr17.specobj and ukidss_dr11plus.dxssource crossmatch (1.5 arcsec)
- sdss_dr17.x1p5__specobj__ukidss_dr11plus__gcssourcesdss_dr17.specobj and ukidss_dr11plus.gcssource crossmatch (1.5 arcsec)
- sdss_dr17.x1p5__specobj__ukidss_dr11plus__gpssourcesdss_dr17.specobj and ukidss_dr11plus.gpssource crossmatch (1.5 arcsec)
- sdss_dr17.x1p5__specobj__ukidss_dr11plus__lassourcesdss_dr17.specobj and ukidss_dr11plus.lassource crossmatch (1.5 arcsec)
- sdss_dr17.x1p5__specobj__ukidss_dr11plus__udssourcesdss_dr17.specobj and ukidss_dr11plus.udssource crossmatch (1.5 arcsec)
- sdss_dr17.x1p5__specobj__unwise_dr1__objectsdss_dr17.specobj and xmatch_std.unwise_dr1__object crossmatch (1.5 arcsec)
- sdss_dr17.x1p5__specobj__usno__a2sdss_dr17.specobj and xmatch_std.usno__a2 crossmatch (1.5 arcsec)
- sdss_dr17.x1p5__specobj__usno__b1sdss_dr17.specobj and xmatch_std.usno__b1 crossmatch (1.5 arcsec)
- sdss_dr17.x1p5__specobj__vhs_dr5__vhs_cat_v3sdss_dr17.specobj and xmatch_std.vhs_dr5__vhs_cat_v3 crossmatch (1.5 arcsec)
- sga2020
- sga2020.ellipseEllipse-fitting results
- sga2020.tractorTractor modeling results
- sga2020.x1p5__tractor__allwise__sourcesga2020.tractor and xmatch_std.allwise__source crossmatch (1.5 arcsec)
- sga2020.x1p5__tractor__gaia_dr3__gaia_sourcesga2020.tractor and gaia_dr3.gaia_source crossmatch (1.5 arcsec)
- sga2020.x1p5__tractor__nsc_dr2__objectsga2020.tractor and xmatch_std.nsc_dr2__object crossmatch (1.5 arcsec)
- sga2020.x1p5__tractor__sdss_dr17__specobjsga2020.tractor and sdss_dr17.specobj crossmatch (1.5 arcsec)
- sga2020.x1p5__tractor__unwise_dr1__objectsga2020.tractor and xmatch_std.unwise_dr1__object crossmatch (1.5 arcsec)
- skymapper_dr1
- skymapper_dr1.mastermean object astrometry, photometry and shape information from all good detections. This table should be used for most photometric queries and is also exposed through the Cone Search service (285,159,194 rows, 100 columns)
- skymapper_dr1.x1p5__master__allwise__sourceskymapper_dr1.master and allwise.source crossmatch (1.5 arcsec)
- skymapper_dr1.x1p5__master__gaia_dr3__gaia_sourceskymapper_dr1.master and gaia_dr3.gaia_source crossmatch (1.5 arcsec)
- skymapper_dr1.x1p5__master__nsc_dr2__objectskymapper_dr1.master and nsc_dr2.object crossmatch (1.5 arcsec)
- skymapper_dr1.x1p5__master__sdss_dr16__specobjskymapper_dr1.master and xmatch_std.sdss_dr16__specobj crossmatch (1.5 arcsec)
- skymapper_dr1.x1p5__master__unwise_dr1__objectskymapper_dr1.master and xmatch_std.unwise_dr1__object crossmatch (1.5 arcsec)
- skymapper_dr2
- skymapper_dr2.masterPrimary table of mean astrometric, photometric and shape measurements per object, with cross-match information to external tables.
- skymapper_dr2.photometryTable of individual photometric, astrometric and shape measurements for every detection. Can be joined to the master table using the object_id column.
- skymapper_dr2.photometry_gTable of individual photometric, astrometric and shape measurements for g-band detections. Can be joined to the master table using the object_id column.
- skymapper_dr2.photometry_iTable of individual photometric, astrometric and shape measurements for i-band detections. Can be joined to the master table using the object_id column.
- skymapper_dr2.photometry_rTable of individual photometric, astrometric and shape measurements for r-band detections. Can be joined to the master table using the object_id column.
- skymapper_dr2.photometry_uTable of individual photometric, astrometric and shape measurements for u-band detections. Can be joined to the master table using the object_id column.
- skymapper_dr2.photometry_vTable of individual photometric, astrometric and shape measurements for v-band detections. Can be joined to the master table using the object_id column.
- skymapper_dr2.photometry_zTable of individual photometric, astrometric and shape measurements for z-band detections. Can be joined to the master table using the object_id column.
- skymapper_dr2.x1p5__master__allwise__sourceskymapper_dr2.master and xmatch_std.allwise__source crossmatch (1.5 arcsec)
- skymapper_dr2.x1p5__master__gaia_dr3__gaia_sourcexmatch_std.skymapper_dr2__master and gaia_dr3.gaia_source crossmatch (1.5 arcsec)
- skymapper_dr2.x1p5__master__nsc_dr2__objectskymapper_dr2.master and xmatch_std.nsc_dr2__object crossmatch (1.5 arcsec)
- skymapper_dr2.x1p5__master__sdss_dr17__specobjxmatch_std.skymapper_dr2__master and sdss_dr17.specobj crossmatch (1.5 arcsec)
- skymapper_dr2.x1p5__master__unwise_dr1__objectskymapper_dr2.master and xmatch_std.unwise_dr1__object crossmatch (1.5 arcsec)
- smash_dr1
- smash_dr1.chipInfo on each chip in the frame
- smash_dr1.exposureInfo on each exposure
- smash_dr1.fieldInfo on each target field (position, Num exposures, etc)
- smash_dr1.galaxiesView of object table to select for galaxies
- smash_dr1.objectAverage photometry of each unique object
- smash_dr1.sourceAll of the individual source measurements
- smash_dr1.starsView of object table to select for stars
- smash_dr1.x1p5__object__gaia_dr3__gaia_sourcesmash_dr1.object and gaia_dr3.gaia_source crossmatch (1.5 arcsec)
- smash_dr1.x1p5__object__nsc_dr2__objectsmash_dr1.object and nsc_dr2.object crossmatch (1.5 arcsec)
- smash_dr1.x1p5__object__unwise_dr1__objectsmash_dr1.object and unwise_dr1.object crossmatch (1.5 arcsec)
- smash_dr1.xmatchCrossmatch of object against GAIA DR1 and WISE
- smash_dr2
- smash_dr2.chipInfo on each chip in the frame
- smash_dr2.deepAverage photometry of each unique object only from deep exposures
- smash_dr2.exposureInfo on each exposure
- smash_dr2.fieldInfo on each target field (position, Num exposures, etc)
- smash_dr2.objectAverage photometry of each unique object
- smash_dr2.sourceAll of the individual source measurements
- smash_dr2.x1p5__object__allwise__sourcesmash_dr2.object and allwise.source crossmatch (1.5 arcsec)
- smash_dr2.x1p5__object__gaia_dr3__gaia_sourcexmatch_std.smash_dr2__object and gaia_dr3.gaia_source crossmatch (1.5 arcsec)
- smash_dr2.x1p5__object__nsc_dr2__objectsmash_dr2.object and nsc_dr2.object crossmatch (1.5 arcsec)
- smash_dr2.x1p5__object__unwise_dr1__objectsmash_dr2.object and unwise_dr1.object crossmatch (1.5 arcsec)
- smash_dr2.xmatchCrossmatch of object against GAIA DR2 and WISE
- sparcl
- splus_dr1
- splus_dr1.des_dr1SPLUS DR1 1.5-arcsec xmatch v. DES DR1
- splus_dr1.stripe82Main S-PLUS object table
- splus_dr1.x1p5__stripe82__allwise__sourcesplus_dr1.stripe82 and allwise.source crossmatch (1.5 arcsec)
- splus_dr1.x1p5__stripe82__gaia_dr3__gaia_sourcesplus_dr1.stripe82 and gaia_dr3.gaia_source crossmatch (1.5 arcsec)
- splus_dr1.x1p5__stripe82__nsc_dr2__objectsplus_dr1.stripe82 and nsc_dr2.object crossmatch (1.5 arcsec)
- splus_dr1.x1p5__stripe82__sdss_dr16__specobjsplus_dr1.stripe82 and sdss_dr16.specobj crossmatch (1.5 arcsec)
- splus_dr1.x1p5__stripe82__unwise_dr1__objectsplus_dr1.stripe82 and unwise_dr1.object crossmatch (1.5 arcsec)
- splus_dr2
- splus_dr2.mainMain object table containing photometry in g, i, r, u, z, f378, f395, f410, f430, f515, f660, and f861 bands.
- splus_dr2.photozPhotometric redshifts table with values obtained via deep-learning using a Mixture Density Network.
- splus_dr2.star_galaxy_quasar_classTable of object classifications and their probabilities. The classification is done using a Random Forest algorithm trained with the 12 S-PLUS bands, FWHM_n, A, B, and KRON_RADIUS.
- splus_dr2.x1p5__main__allwise__sourcesplus_dr2.main and xmatch_std.allwise__source crossmatch (1.5 arcsec)
- splus_dr2.x1p5__main__gaia_dr3__gaia_sourcexmatch_std.splus_dr2__main and gaia_dr3.gaia_source crossmatch (1.5 arcsec)
- splus_dr2.x1p5__main__nsc_dr2__objectsplus_dr2.main and xmatch_std.nsc_dr2__object crossmatch (1.5 arcsec)
- splus_dr2.x1p5__main__sdss_dr17__specobjxmatch_std.splus_dr2__main and sdss_dr17.specobj crossmatch (1.5 arcsec)
- splus_dr2.x1p5__main__unwise_dr1__objectsplus_dr2.main and xmatch_std.unwise_dr1__object crossmatch (1.5 arcsec)
- splus_edr
- splus_edr.des_dr1SPLUS EDR 1.5-arcsec xmatch v. DES DR1
- splus_edr.stripe82Main S-PLUS object table
- splus_edr.x1p5__stripe82__allwise__sourcesplus_edr.stripe82 and allwise.source crossmatch (1.5 arcsec)
- splus_edr.x1p5__stripe82__gaia_dr3__gaia_sourcesplus_edr.stripe82 and gaia_dr3.gaia_source crossmatch (1.5 arcsec)
- splus_edr.x1p5__stripe82__nsc_dr2__objectsplus_edr.stripe82 and nsc_dr2.object crossmatch (1.5 arcsec)
- splus_edr.x1p5__stripe82__sdss_dr17__specobjsplus_edr.stripe82 and sdss_dr17.specobj crossmatch (1.5 arcsec)
- splus_edr.x1p5__stripe82__unwise_dr1__objectsplus_edr.stripe82 and unwise_dr1.object crossmatch (1.5 arcsec)
- stripe82
- stripe82.allwiseAllWISE Source Table
- stripe82.des_dr1Dark Energy Survey (DES) Data Release 1
- stripe82.gaia_dr1Gaia Data Release 1
- stripe82.gaia_dr2Gaia Data Release 2
- stripe82.nsc_dr1NOAO Source Catalog Release 1
- stripe82.sdss13_specobjSDSS DR13 specobj table
- stripe82.sdss14_specobjSDSS DR14 specobj table
- stripe82.splus_dr1SPLUS DR1 Object Table
- stripe82.twomass_psc2MASS Point Source Catalog
- stripe82.twomass_xsc2MASS Extended Source Catalog
- stripe82.usno_a2USNO-A2
- stripe82.usno_b1USNO-B1
- tap_schema
- twomass
- twomass.pscPoint Source Catalog (470,992,970 rows)
- twomass.x1p5__psc__allwise__sourcetwomass.psc and allwise.source crossmatch (1.5 arcsec)
- twomass.x1p5__psc__gaia_dr3__gaia_sourcexmatch_std.twomass__psc and gaia_dr3.gaia_source crossmatch (1.5 arcsec)
- twomass.x1p5__psc__nsc_dr2__objecttwomass.psc and nsc_dr2.object crossmatch (1.5 arcsec)
- twomass.x1p5__psc__sdss_dr17__specobjxmatch_std.twomass__psc and sdss_dr17.specobj crossmatch (1.5 arcsec)
- twomass.x1p5__psc__unwise_dr1__objecttwomass.psc and xmatch_std.unwise_dr1 crossmatch (1.5 arcsec)
- twomass.x1p5__xsc__allwise__sourcetwomass.xsc and allwise.source crossmatch (1.5 arcsec)
- twomass.x1p5__xsc__gaia_dr3__gaia_sourcexmatch_std.twomass__xsc and gaia_dr3.gaia_source crossmatch (1.5 arcsec)
- twomass.x1p5__xsc__nsc_dr1__objecttwomass.xsc and nsc_dr1.object crossmatch (1.5 arcsec)
- twomass.x1p5__xsc__nsc_dr2__objecttwomass.xsc and nsc_dr2.object crossmatch (1.5 arcsec)
- twomass.x1p5__xsc__sdss_dr17__specobjxmatch_std.twomass__xsc and sdss_dr17.specobj crossmatch (1.5 arcsec)
- twomass.x1p5__xsc__unwise_dr1__objecttwomass.xsc and unwise_dr1.object crossmatch (1.5 arcsec)
- twomass.xscExtended Source Catalog (1,647,599 rows)
- tycho2
- tycho2.mainThe Tycho-2 main catalogue
- tycho2.x1p5__main__allwise__sourcetycho2.main and allwise.source crossmatch (1.5 arcsec)
- tycho2.x1p5__main__gaia_dr3__gaia_sourcetycho2.main and gaia_dr3.gaia_source crossmatch (1.5 arcsec)
- tycho2.x1p5__main__nsc_dr1__objecttycho2.main and nsc_dr1.object crossmatch (1.5 arcsec)
- tycho2.x1p5__main__sdss_dr17__specobjtycho2.main and sdss_dr17.specobj crossmatch (1.5 arcsec)
- tycho2.x1p5__main__unwise_dr1__objecttycho2.main and unwise_dr1.object crossmatch (1.5 arcsec)
- ukidss_dr11plus
- ukidss_dr11plus.dxssourceDeep Extragalactic Survey (DXS) 35 sq.deg. K=21 on completion. Longer exposures, and stacked over many nights.
- ukidss_dr11plus.gcssourceGalactic Cluster Survey (GCS) on completion, 1000 sq. deg. to K=18.7. Short exposures, unstacked, but later 2nd pass.
- ukidss_dr11plus.gpssourceGalactic Plane Survey (GPS) on completion, 1800 sq.deg. to K=19.0. Main survey : short exposures, unstacked, but later 2nd pass. Some deeper stacked sub-components.
- ukidss_dr11plus.lassourceLarge Area Survey (LAS) : on completion, 4000 sq.deg. to K=18.4. Short exposures, unstacked, but later 2nd pass.
- ukidss_dr11plus.udssourceUltra Deep Survey (UDS) : 0.75 sq.deg. K=23 on completion. Very long exposure, stacked over many many nights.
- ukidss_dr11plus.x1p5__dxssource__allwise__sourceukidss_dr11plus.dxssource and xmatch_std.allwise__source crossmatch (1.5 arcsec)
- ukidss_dr11plus.x1p5__dxssource__gaia_dr3__gaia_sourceukidss_dr11plus.dxssource and gaia_dr3.gaia_source crossmatch (1.5 arcsec)
- ukidss_dr11plus.x1p5__dxssource__nsc_dr2__objectukidss_dr11plus.dxssource and xmatch_std.nsc_dr2__object crossmatch (1.5 arcsec)
- ukidss_dr11plus.x1p5__dxssource__sdss_dr17__specobjukidss_dr11plus.dxssource and sdss_dr17.specobj crossmatch (1.5 arcsec)
- ukidss_dr11plus.x1p5__dxssource__unwise_dr1__objectukidss_dr11plus.dxssource and xmatch_std.unwise_dr1__object crossmatch (1.5 arcsec)
- ukidss_dr11plus.x1p5__gcssource__allwise__sourceukidss_dr11plus.gcssource and xmatch_std.allwise__source crossmatch (1.5 arcsec)
- ukidss_dr11plus.x1p5__gcssource__gaia_dr3__gaia_sourceukidss_dr11plus.gcssource and gaia_dr3.gaia_source crossmatch (1.5 arcsec)
- ukidss_dr11plus.x1p5__gcssource__nsc_dr2__objectukidss_dr11plus.gcssource and xmatch_std.nsc_dr2__object crossmatch (1.5 arcsec)
- ukidss_dr11plus.x1p5__gcssource__sdss_dr17__specobjukidss_dr11plus.gcssource and sdss_dr17.specobj crossmatch (1.5 arcsec)
- ukidss_dr11plus.x1p5__gcssource__unwise_dr1__objectukidss_dr11plus.gcssource and xmatch_std.unwise_dr1__object crossmatch (1.5 arcsec)
- ukidss_dr11plus.x1p5__gpssource__allwise__sourceukidss_dr11plus.gpssource and xmatch_std.allwise__source crossmatch (1.5 arcsec)
- ukidss_dr11plus.x1p5__gpssource__gaia_dr3__gaia_sourceukidss_dr11plus.gpssource and gaia_dr3.gaia_source crossmatch (1.5 arcsec)
- ukidss_dr11plus.x1p5__gpssource__nsc_dr2__objectukidss_dr11plus.gpssource and xmatch_std.nsc_dr2__object crossmatch (1.5 arcsec)
- ukidss_dr11plus.x1p5__gpssource__sdss_dr17__specobjukidss_dr11plus.gpssource and sdss_dr17.specobj crossmatch (1.5 arcsec)
- ukidss_dr11plus.x1p5__gpssource__unwise_dr1__objectukidss_dr11plus.gpssource and xmatch_std.unwise_dr1__object crossmatch (1.5 arcsec)
- ukidss_dr11plus.x1p5__lassource__allwise__sourceukidss_dr11plus.lassource and xmatch_std.allwise__source crossmatch (1.5 arcsec)
- ukidss_dr11plus.x1p5__lassource__gaia_dr3__gaia_sourceukidss_dr11plus.lassource and gaia_dr3.gaia_source crossmatch (1.5 arcsec)
- ukidss_dr11plus.x1p5__lassource__nsc_dr2__objectukidss_dr11plus.lassource and xmatch_std.nsc_dr2__object crossmatch (1.5 arcsec)
- ukidss_dr11plus.x1p5__lassource__sdss_dr17__specobjukidss_dr11plus.lassource and sdss_dr17.specobj crossmatch (1.5 arcsec)
- ukidss_dr11plus.x1p5__lassource__unwise_dr1__objectukidss_dr11plus.lassource and xmatch_std.unwise_dr1__object crossmatch (1.5 arcsec)
- ukidss_dr11plus.x1p5__udssource__allwise__sourceukidss_dr11plus.udssource and xmatch_std.allwise__source crossmatch (1.5 arcsec)
- ukidss_dr11plus.x1p5__udssource__gaia_dr3__gaia_sourceukidss_dr11plus.udssource and gaia_dr3.gaia_source crossmatch (1.5 arcsec)
- ukidss_dr11plus.x1p5__udssource__nsc_dr2__objectukidss_dr11plus.udssource and xmatch_std.nsc_dr2__object crossmatch (1.5 arcsec)
- ukidss_dr11plus.x1p5__udssource__sdss_dr17__specobjukidss_dr11plus.udssource and sdss_dr17.specobj crossmatch (1.5 arcsec)
- ukidss_dr11plus.x1p5__udssource__unwise_dr1__objectukidss_dr11plus.udssource and xmatch_std.unwise_dr1__object crossmatch (1.5 arcsec)
- unwise_dr1
- unwise_dr1.objectMost columns in the unWISE band-merged catalogs are identical to the individual-image catalogs, and include W1 and W2 measurements of a source.
- unwise_dr1.x1p5__object__allwise__sourceunwise_dr1.object and allwise.source crossmatch (1.5 arcsec)
- unwise_dr1.x1p5__object__catwise2020__mainxmatch_std.unwise_dr1__object and catwise2020.main crossmatch (1.5 arcsec)
- unwise_dr1.x1p5__object__decaps_dr1__objectunwise_dr1.object and decaps_dr1.object crossmatch (1.5 arcsec)
- unwise_dr1.x1p5__object__decaps_dr2__objectxmatch_std.unwise_dr1__object and decaps_dr2.object crossmatch (1.5 arcsec)
- unwise_dr1.x1p5__object__delve_dr1__objectsunwise_dr1.object and delve_dr1.objects crossmatch (1.5 arcsec)
- unwise_dr1.x1p5__object__delve_dr2__objectsxmatch_std.unwise_dr1__object and delve_dr2.objects crossmatch (1.5 arcsec)
- unwise_dr1.x1p5__object__des_dr1__mainunwise_dr1.object and des_dr1.main crossmatch (1.5 arcsec)
- unwise_dr1.x1p5__object__des_dr2__mainunwise_dr1.object and des_dr2.main crossmatch (1.5 arcsec)
- unwise_dr1.x1p5__object__desi_edr__zpixxmatch_std.unwise_dr1__object and desi_edr.zpix crossmatch (1.5 arcsec)
- unwise_dr1.x1p5__object__gaia_dr1__gaia_sourceunwise_dr1.object and gaia_dr1.gaia_source crossmatch (1.5 arcsec)
- unwise_dr1.x1p5__object__gaia_dr2__gaia_sourceunwise_dr1.object and gaia_dr2.gaia_source crossmatch (1.5 arcsec)
- unwise_dr1.x1p5__object__gaia_dr3__gaia_sourcexmatch_std.unwise_dr1__object and gaia_dr3.gaia_source crossmatch (1.5 arcsec)
- unwise_dr1.x1p5__object__gnirs_dqs__spec_measurementsxmatch_std.unwise_dr1__object and gnirs_dqs.spec_measurements crossmatch (1.5 arcsec)
- unwise_dr1.x1p5__object__gogreen_dr1__photounwise_dr1.object and gogreen_dr1.photo crossmatch (1.5 arcsec)
- unwise_dr1.x1p5__object__gogreen_dr1__redshiftunwise_dr1.object and gogreen_dr1.redshift crossmatch (1.5 arcsec)
- unwise_dr1.x1p5__object__ls_dr10__tractorxmatch_std.unwise_dr1__object and ls_dr10.tractor crossmatch (1.5 arcsec)
- unwise_dr1.x1p5__object__ls_dr8__tractorxmatch_std.unwise_dr1__object and ls_dr8.tractor crossmatch (1.5 arcsec)
- unwise_dr1.x1p5__object__ls_dr9__tractorxmatch_std.unwise_dr1__object and xmatch_std.ls_dr9__tractor crossmatch (1.5 arcsec)
- unwise_dr1.x1p5__object__nsc_dr2__objectunwise_dr1.object and nsc_dr2.object crossmatch (1.5 arcsec)
- unwise_dr1.x1p5__object__phat_v2__phot_modunwise_dr1.object and phat_v2.phot_mod crossmatch (1.5 arcsec)
- unwise_dr1.x1p5__object__sdss_dr12__specobjunwise_dr1.object and sdss_dr12.specobj crossmatch (1.5 arcsec)
- unwise_dr1.x1p5__object__sdss_dr13__specobjunwise_dr1.object and sdss_dr13.specobj crossmatch (1.5 arcsec)
- unwise_dr1.x1p5__object__sdss_dr14__specobjunwise_dr1.object and sdss_dr14.specobj crossmatch (1.5 arcsec)
- unwise_dr1.x1p5__object__sdss_dr16__specobjunwise_dr1.object and sdss_dr16.specobj crossmatch (1.5 arcsec)
- unwise_dr1.x1p5__object__sdss_dr17__specobjxmatch_std.unwise_dr1__object and sdss_dr17.specobj crossmatch (1.5 arcsec)
- unwise_dr1.x1p5__object__sga2020__tractorxmatch_std.unwise_dr1__object and sga2020.tractor crossmatch (1.5 arcsec)
- unwise_dr1.x1p5__object__skymapper_dr1__masterxmatch_std.unwise_dr1__object and skymapper_dr1.master crossmatch (1.5 arcsec)
- unwise_dr1.x1p5__object__skymapper_dr2__masterxmatch_std.unwise_dr1__object and skymapper_dr2.master crossmatch (1.5 arcsec)
- unwise_dr1.x1p5__object__smash_dr1__objectunwise_dr1.object and smash_dr1.object crossmatch (1.5 arcsec)
- unwise_dr1.x1p5__object__smash_dr2__objectunwise_dr1.object and smash_dr2.object crossmatch (1.5 arcsec)
- unwise_dr1.x1p5__object__splus_dr1__stripe82unwise_dr1.object and splus_dr1.stripe82 crossmatch (1.5 arcsec)
- unwise_dr1.x1p5__object__splus_dr2__mainxmatch_std.unwise_dr1__object and splus_dr2.main crossmatch (1.5 arcsec)
- unwise_dr1.x1p5__object__splus_edr__stripe82unwise_dr1.object and splus_edr.stripe82 crossmatch (1.5 arcsec)
- unwise_dr1.x1p5__object__twomass__pscunwise_dr1.object and twomass.psc crossmatch (1.5 arcsec)
- unwise_dr1.x1p5__object__twomass__xscunwise_dr1.object and twomass.xsc crossmatch (1.5 arcsec)
- unwise_dr1.x1p5__object__tycho2__mainunwise_dr1.object and tycho2.main crossmatch (1.5 arcsec)
- unwise_dr1.x1p5__object__ukidss_dr11plus__dxssourcexmatch_std.unwise_dr1__object and ukidss_dr11plus.dxssource crossmatch (1.5 arcsec)
- unwise_dr1.x1p5__object__ukidss_dr11plus__gcssourcexmatch_std.unwise_dr1__object and ukidss_dr11plus.gcssource crossmatch (1.5 arcsec)
- unwise_dr1.x1p5__object__ukidss_dr11plus__gpssourcexmatch_std.unwise_dr1__object and ukidss_dr11plus.gpssource crossmatch (1.5 arcsec)
- unwise_dr1.x1p5__object__ukidss_dr11plus__lassourcexmatch_std.unwise_dr1__object and ukidss_dr11plus.lassource crossmatch (1.5 arcsec)
- unwise_dr1.x1p5__object__ukidss_dr11plus__udssourcexmatch_std.unwise_dr1__object and ukidss_dr11plus.udssource crossmatch (1.5 arcsec)
- unwise_dr1.x1p5__object__usno__a2unwise_dr1.object and usno.a2 crossmatch (1.5 arcsec)
- unwise_dr1.x1p5__object__usno__b1unwise_dr1.object and usno.b1 crossmatch (1.5 arcsec)
- unwise_dr1.x1p5__object__vhs_dr5__vhs_cat_v3unwise_dr1.object and vhs_dr5.vhs_cat_v3 crossmatch (1.5 arcsec)
- usno
- usno.a2USNO-A2 catalog
- usno.b1USNO-B1 catalog
- usno.x1p5__a2__allwise__sourceusno.a2 and allwise.source crossmatch (1.5 arcsec)
- usno.x1p5__a2__gaia_dr3__gaia_sourcexmatch_std.usno__a2 and gaia_dr3.gaia_source crossmatch (1.5 arcsec)
- usno.x1p5__a2__nsc_dr2__objectusno.a2 and nsc_dr2.object crossmatch (1.5 arcsec)
- usno.x1p5__a2__sdss_dr17__specobjxmatch_std.usno__a2 and sdss_dr17.specobj crossmatch (1.5 arcsec)
- usno.x1p5__a2__unwise_dr1__objectusno.a2 and unwise_dr1.object crossmatch (1.5 arcsec)
- usno.x1p5__b1__allwise__sourceusno.b1 and allwise.source crossmatch (1.5 arcsec)
- usno.x1p5__b1__gaia_dr3__gaia_sourcexmatch_std.usno__b1 and gaia_dr3.gaia_source crossmatch (1.5 arcsec)
- usno.x1p5__b1__nsc_dr2__objectusno.b1 and nsc_dr2.object crossmatch (1.5 arcsec)
- usno.x1p5__b1__sdss_dr17__specobjxmatch_std.usno__b1 and sdss_dr17.specobj crossmatch (1.5 arcsec)
- usno.x1p5__b1__unwise_dr1__objectusno.b1 and unwise_dr1.object crossmatch (1.5 arcsec)
- vhs_dr5
- vhs_dr5.vhs_cat_v3This multi-band source catalogue provides aperture photometry in four near infrared broad-band filters: Y, J, H and Ks for almost 1.4 billion detections. The total coverage of the VHS survey is almost 17000 square degrees in the South Hemisphere.
- vhs_dr5.x1p5__vhs_cat_v3__allwise__sourcevhs_dr5.vhs_cat_v3 and allwise.source crossmatch (1.5 arcsec)
- vhs_dr5.x1p5__vhs_cat_v3__gaia_dr3__gaia_sourcexmatch_std.vhs_dr5__vhs_cat_v3 and gaia_dr3.gaia_source crossmatch (1.5 arcsec)
- vhs_dr5.x1p5__vhs_cat_v3__nsc_dr2__objectvhs_dr5.vhs_cat_v3 and nsc_dr2.object crossmatch (1.5 arcsec)
- vhs_dr5.x1p5__vhs_cat_v3__sdss_dr17__specobjxmatch_std.vhs_dr5__vhs_cat_v3 and sdss_dr17.specobj crossmatch (1.5 arcsec)
- vhs_dr5.x1p5__vhs_cat_v3__unwise_dr1__objectvhs_dr5.vhs_cat_v3 and unwise_dr1.object crossmatch (1.5 arcsec)
- SIA tables
- ivoa_calibrated
- ivoa_calibrated.calibrated_allAll instrument calibrated images
- ivoa_calibrated.des_y1Instrument calibrated images from the Dark Energy Survey DR1 obtained in the first year of DES
- ivoa_calibrated.des_y2Instrument calibrated images from the Dark Energy Survey DR1 obtained in the second year of DES
- ivoa_calibrated.des_y3Instrument calibrated images from the Dark Energy Survey DR1 obtained in the third year of DES
- ivoa_calibrated.des_y4Instrument calibrated images from the Dark Energy Survey DR1 obtained in the fourth year of DES
- ivoa_calibrated.nsaInstrument calibrated images from the Astro Data Archive
- ivoa_calibrated.smash_dr1Instrument calibrated images from SMASH DR1
- ivoa_calibrated.smash_dr2Instrument calibrated images from SMASH DR2
- ivoa_calibrated.splus_dr1Instrument calibrated images from S-PLUS DR1
- ivoa_coadd
- ivoa_coadd.coadd_allStacked calibrated images from all surveys
- ivoa_coadd.decaps_dr1Stacked calibrated images from DECaPS DR1
- ivoa_coadd.des_dr1Stacked calibrated images from the Dark Energy Survey DR1
- ivoa_coadd.des_svaStacked calibrated images from the Dark Energy Survey SVA
- ivoa_coadd.ls_dr8Stacked calibrated images from Legacy Surveys DR8
- ivoa_coadd.ls_dr9Stacked calibrated images from Legacy Surveys DR9
- ivoa_coadd.nsaStacked calibrated images from the Astro Data Archive
- ivoa_coadd.smash_dr1Stacked calibrated images from SMASH DR1
- ivoa_coadd.smash_dr2Stacked calibrated images from SMASH DR2
- ivoa_coadd.splus_dr1Stacked calibrated images from S-PLUS DR1
- ivoa_decaps_dr1
- ivoa_des_dr1
- ivoa_des_dr2
- ivoa_des_dr2_se
- ivoa_des_sva1
- ivoa_des_y1
- ivoa_des_y2
- ivoa_des_y3
- ivoa_des_y4
- ivoa_gogreen_dr1
- ivoa_ls_dr8
- ivoa_ls_dr9
- ivoa_nsa
- ivoa_nsc_dr2
- ivoa_raw
- ivoa_sdss_dr9
- ivoa_smash_dr1
- ivoa_smash_dr2
- ivoa_splus_dr1
- ivoa_splus_edr
- ivoa_stripe82
- ivoa_stripe82.calibratedInstrument calibrated images that overlap with SDSS Stripe 82
- ivoa_stripe82.coaddStacked calibrated images that overlap with SDSS Stripe 82
- ivoa_stripe82.decaps_dr1Images from DECaPS DR1 that overlap with SDSS Stripe 82
- ivoa_stripe82.des_dr1Images from the Dark Energy Survey DR1 that overlap with SDSS Stripe 82
- ivoa_stripe82.des_dr2Images from the Dark Energy Survey DR2 that overlap with SDSS Stripe 82
- ivoa_stripe82.des_sva1Images from the Dark Energy Survey SVA1 that overlap with SDSS Stripe 82
- ivoa_stripe82.des_y1Images from the Dark Energy Survey DR1 obtained in the first year of DES that overlap with SDSS Stripe 82
- ivoa_stripe82.des_y2Images from the Dark Energy Survey DR1 obtained in the second year of DES that overlap with SDSS Stripe 82
- ivoa_stripe82.des_y3Images from the Dark Energy Survey DR1 obtained in the third year of DES that overlap with SDSS Stripe 82
- ivoa_stripe82.des_y4Images from the Dark Energy Survey DR1 obtained in the fourth year of DES that overlap with SDSS Stripe 82
- ivoa_stripe82.ls_dr8Images from Legacy Surveys DR8 that overlap with SDSS Stripe 82
- ivoa_stripe82.ls_dr9Images from Legacy Surveys DR9 that overlap with SDSS Stripe 82
- ivoa_stripe82.nsaImages from the Astro Data Archive that overlap with SDSS Stripe 82
- ivoa_stripe82.nsc_dr2Images from NSC DR2 that overlap with SDSS Stripe 82
- ivoa_stripe82.rawRaw uncalibrated images that overlap with SDSS Stripe 82
- ivoa_stripe82.sdss_dr9Images from SDSS DR9 that overlap with SDSS Stripe 82
- ivoa_stripe82.smash_dr1Images from SMASH DR1 that overlap with SDSS Stripe 82
- ivoa_stripe82.smash_dr2Images from SMASH DR2 that overlap with SDSS Stripe 82
- ivoa_stripe82.splus_dr1Images from S-PLUS DR1 that overlap with SDSS Stripe 82
- ivoa_stripe82.splus_edrImages from S-PLUS EDR that overlap with SDSS Stripe 82
- ivoa_stripe82.stripe82_allImages from all surveys that overlap with SDSS Stripe 82
- ivoa_calibrated
The Astro Data Lab is part of the Community Science and Data Center (CSDC) at NSF’s NOIRLab, the national center for ground-based nighttime astronomy in the United States operated by the Association of Universities for Research in Astronomy (AURA) under cooperative agreement with the National Science Foundation.
For further information, contact datalab@noirlab.edu.
- Design: Wendy Huang, Mark Newhouse & HTML5 UP