J/A+A/664/A126ivo://CDS.VizieR/J/A+A/664/A126doi:10.26093/cds/vizier.36640126CDSLiu T.Merloni A.Wolf J.Salvato M.Reiprich T.H.Comparat J.,Arcodia R.Lamer G.Georgakakis A.Dwelly T.Sanders J.Buchner J.,Haberl F.Ramos-Ceja M.E.Wilms J.Nandra K.Brunner H.Brusa M.,Schwope A.Robrade J.Freyberg M.Boller T.Maitra C.Veronica A.,Malyali A.2023-03-20T14:04:33Z2022-08-18T12:30:17ZCDS support team

CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France

cds-question@unistra.frx-ray-sourcessurveysThe eROSITA X-ray telescope on board the SRG observatory performed Calibration and Performance Verification (CalPV) observations between September 2019 and December 2019, ahead of the planned four-year all-sky surveys. Most of them were deep, pointing-mode observations. We present here the X-ray catalog detected from the set of extra-galactic CalPV observations released to the public by the German eROSITA consortium, and the multi-band counterparts of these X-ray sources. We develop a source detection method optimized for point-like X-ray sources by including extended X-ray emission in the background measurement. The multi-band counterparts are identified using a Bayesian method from the CatWISE catalog. Combining 11 CalPV fields, we present a catalog containing 9522 X-ray sources, whose X-ray fluxes are measured through spectral fitting. CatWISE counterparts are presented for 77% of the sources. Significant variabilities are found in 99 of the sources, which are also presented with this paper. Most of these fields show similar number counts of point sources as typical extragalactic fields, and a few harbor particular stellar populations.2022A&A...664A.126Lhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/664/A126CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toJ/A+A/661/A1 : The eFEDS X-ray catalogs (V7.4) (Brunner+, 2022)J/A+A/661/A2 : Galaxy clusters and groups in eFEDS (Liu+, 2022)J/A+A/661/A3 : eFEDS counterparts to point-like sources (Salvato+, 2022)J/A+A/661/A4 : eFEDS optical cluster and group catalog (Klein+, 2022)J/A+A/661/A5 : The eFEDS AGN catalog (Liu+, 2022)J/A+A/661/A7 : X-ray properties of eFEDS clusters and groups (Bahar+, 2022)J/A+A/661/A8 : eFEDS catalogue of variable X-ray sources (Boller+, 2022)J/A+A/661/A10 : eFEDS galaxy clusters and groups in disguise (Bulbul+, 2022)J/A+A/661/A23 : Exoplanet X-ray irradiation & evaporation rates (Foster+, 2022)J/A+A/661/A24 : Corona-chromosphere connection (Fuhrmeister+, 2022)J/A+A/661/A29 : First eROSITA study of nearby M dwarfs (Magaudda+, 2022)J/A+A/661/A34 : eta Cha cluster eROSITA X-ray scan (Robrade+, 2022)J/A+A/661/A35 : eROSITA study of 47 Tuc globular cluster (Saeedi+, 2022)J/A+A/661/A38 : SRG/ART-XC 1st year all-sky X-ray survey (Pavlinsky+, 2022)J/A+A/661/A40 : eRASS1 X-ray sources Sco-Cen members (Schmitt+, 2022)J/A+A/661/A44 : A first eROSITA view of ultracool dwarfs (Stelzer+, 2022)https://erosita.mpe.mpg.de/edr/eROSITAObservations/Catalogues/liuT/CalPVexG_V1.html : CalPV Home Pagehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/664/A126https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/664/A126http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/664/A126https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/664/A126https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/664/A126http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/664/A126GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/A+A/664/A126/calpvexg (The eROSITA extragalactic CalPV serendipitous X-ray catalog, converted from CalPVexG_V3.3.fits)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/664/A126/calpvexg?https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/664/A126/calpvexg?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/664/A126/calpvexg?GETtext/xml+votable180.050000true107.1728855215945-49.55207587220710.005555555555555556Cone search capability for table J/A+A/664/A126/calpvctp (The counterparts of the X-ray sources, converted from CalPVexG_CTP_V3.3.fits)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/664/A126/calpvctp?https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/664/A126/calpvctp?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/664/A126/calpvctp?GETtext/xml+votable180.050000true107.1046275150835-49.19999478303530.0055555555555555565/9766 9769 9771 6/16295 16301 16306 16312 16435 16438 16441 16443-16444 33234-33235 33240-33241 33306-33307 33315 33317-33319 33321 33323-33324 33326 33328-33330 33625 33627-33628 33630 39053-39055 39058-39059 39088-39090 39096 39118 39137 39140 39428 46362-46363 46384-46385 47738-47739 47742 47813 47824-47826 47828https://cdsarc.cds.unistra.fr/viz-bin/moc/J/A+A/664/A126?format=asciiX-raydefaultJ/A+A/664/A126/calpvexgThe eROSITA extragalactic CalPV serendipitous X-ray catalog, converted from CalPVexG_V3.3.fitsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintMoreindicates counterparts and/or variable in other tablesmeta.ref.urlcharNameSource name (Name)meta.id;meta.maincharUIDUnique source ID (UID)meta.idcharprimaryFieldField name (Field)meta.id;obs.fieldcharID-SRC[1/2795] Source ID in each field (ID_SRC)meta.idintinMskPnt[0/1] Whether in the point-source sub-survey region (inMskPnt)meta.codeintRAcdegRight ascension (ICRS), corrected using CatWISE2020 (RA_corr)degpos.eq.raDEcdegDeclination (ICRS), corrected using CatWISE2020 (DEC_corr)degpos.eq.decePoscCombined positional uncertainty, corrected [arcsec] (RADEC_ERR_corr)arcsecstat.error;posdoubleRAJ2000Uncorrected right ascension (J2000) (RA)degpos.eq.ra;meta.maine_RAJ2000? 1 sigma RA lower error (RA_LOWERR)arcsecstat.error;pos.eq.radoublenullableE_RAJ2000? 1 sigma RA upper error (RA_UPERR)arcsecstat.error;stat.maxdoublenullableDEJ2000Uncorrected declination (J2000) (DEC)degpos.eq.dec;meta.maine_DEJ2000? 1 sigma DEC lower error (DEC_LOWERR)arcsecstat.error;pos.eq.decdoublenullableE_DEJ2000? 1 sigma DEC upper error (DEC_UPERR)arcsecstat.error;stat.maxdoublenullableePosCombined positional uncertainty, uncorrected (RADEC_ERR)arcsecstat.error;posdoubleDetLike0Detection likelihood, combining bands 1,2,3 (DET_LIKE_0)stat.likelihooddoubleDetLike1Detection likelihood, band 1 (DET_LIKE_1)stat.likelihooddoubleDetLike2Detection likelihood, band 2 (DET_LIKE_2)stat.likelihooddoubleDetLike3Detection likelihood, band 3 (DET_LIKE_3)stat.likelihooddoubleExtSource extent (EXT)arcsecphys.angSizedoubles_Ext? Extent error (EXT_ERR)arcsecstat.error;phys.angSizedoublenullablee_Ext? 1 sigma extent lower error (EXT_LOWERR)arcsecstat.errordoublenullableE_Ext? 1 sigma extent upper error (EXT_UPERR)arcsecstat.error;stat.maxdoublenullableExtLikeExtent likelihood (EXT_LIKE)stat.likelihooddoubleECF-0.5-2sEnergy conversion factor between ML_FLUX_s and ML_RATE_s (in cm^2^/erg) (ECF_0d5_2_s)1e+07cm**2.J**-1instr.paramdoubleECF-2.3-5hEnergy conversion factor between ML_FLUX_h and ML_RATE_t (in cm^2^/erg) (ECF_2d3_5_h)1e+07cm**2.J**-1instr.paramdoubleMLCts1Source net counts measured from count rate (ML_CTS_1)ctphot.countdoubles_MLCts1? 1 sigma counts error (ML_CTS_ERR_1)ctstat.error;phot.countdoublenullablee_MLCts1? 1 sigma counts lower error (ML_CTS_LOWERR_1)ctstat.errordoublenullableE_MLCts1? 1 sigma counts upper error (ML_CTS_UPERR_1)ctstat.error;stat.maxdoublenullableMLRate1Source count rate measured by PSF-fitting (ML_RATE_1)ct/sphot.count;em.X-raydoubles_MLRate1? 1 sigma count rate error (ML_RATE_ERR_1)ct/sarith.rate;phot.countdoublenullablee_MLRate1? 1 sigma count rate lower error (ML_RATE_LOWERR_1)ct/sstat.errordoublenullableE_MLRate1? 1 sigma count rate upper error (ML_RATE_UPERR_1)ct/sstat.error;stat.maxdoublenullableMLFlux1Source flux converted from count rate (ML_FLUX_1)mW.m**-2phot.flux;em.X-raydoubles_MLFlux1? 1 sigma flux error (ML_FLUX_ERR_1)mW.m**-2stat.error;phot.fluxdoublenullablee_MLFlux1? 1 sigma flux lower error (ML_FLUX_LOWERR_1)mW.m**-2stat.errordoublenullableE_MLFlux1? 1 sigma flux upper error (ML_FLUX_UPERR_1)mW.m**-2stat.error;stat.maxdoublenullableMLBkg1Background flux at the source position (ML_BKG_1)arcmin**-2instr.backgrounddoubleMLExp1Vignetted exposure value (ML_EXP_1)sstat.value;obs.exposuredoubleMLEEF1Enclosed energy fraction in the fitting aperture for band 1 PSF (ML_EEF_1)instr.det.psfdoubleMLCts2Source net counts measured from count rate (ML_CTS_2)ctphot.countdoubles_MLCts2? 1 sigma counts error (ML_CTS_ERR_2)ctstat.error;phot.countdoublenullablee_MLCts2? 1 sigma counts lower error (ML_CTS_LOWERR_2)ctstat.errordoublenullableE_MLCts2? 1 sigma counts upper error (ML_CTS_UPERR_2)ctstat.error;stat.maxdoublenullableMLRate2Source count rate measured by PSF-fitting (ML_RATE_2)ct/sphot.count;em.X-raydoubles_MLRate2? 1 sigma count rate error (ML_RATE_ERR_2)ct/sarith.rate;phot.countdoublenullablee_MLRate2? 1 sigma count rate lower error (ML_RATE_LOWERR_2)ct/sstat.errordoublenullableE_MLRate2? 1 sigma count rate upper error (ML_RATE_UPERR_2)ct/sstat.error;stat.maxdoublenullableMLFlux2Source flux converted from count rate (ML_FLUX_2)mW.m**-2phot.flux;em.X-raydoubles_MLFlux2? 1 sigma flux error (ML_FLUX_ERR_2)mW.m**-2stat.error;phot.fluxdoublenullablee_MLFlux2? 1 sigma flux lower error (ML_FLUX_LOWERR_2)mW.m**-2stat.errordoublenullableE_MLFlux2? 1 sigma flux upper error (ML_FLUX_UPERR_2)mW.m**-2stat.error;stat.maxdoublenullableMLBkg2Background flux at the source position (ML_BKG_2)arcmin**-2instr.backgrounddoubleMLExp2Vignetted exposure value (ML_EXP_2)sstat.value;obs.exposuredoubleMLEEF2Enclosed energy fraction in the fitting aperture for band 2 PSF (ML_EEF_2)instr.det.psfdoubleMLCts3Source net counts measured from count rate (ML_CTS_3)ctphot.countdoubles_MLCts3? 1 sigma counts error (ML_CTS_ERR_3)ctstat.error;phot.countdoublenullablee_MLCts3? 1 sigma counts lower error (ML_CTS_LOWERR_3)ctstat.errordoublenullableE_MLCts3? 1 sigma counts upper error (ML_CTS_UPERR_3)ctstat.error;stat.maxdoublenullableMLRate3? Source count rate measured by PSF-fitting (ML_RATE_3)ct/sphot.count;em.X-raydoublenullables_MLRate3? 1 sigma count rate error (ML_RATE_ERR_3)ct/sarith.rate;phot.countdoublenullablee_MLRate3? 1 sigma count rate lower error (ML_RATE_LOWERR_3)ct/sstat.errordoublenullableE_MLRate3? 1 sigma count rate upper error (ML_RATE_UPERR_3)ct/sstat.error;stat.maxdoublenullableMLFlux3? Source flux converted from count rate (ML_FLUX_3)mW.m**-2phot.flux;em.X-raydoublenullables_MLFlux3? 1 sigma flux error (ML_FLUX_ERR_3)mW.m**-2stat.error;phot.fluxdoublenullablee_MLFlux3? 1 sigma flux lower error (ML_FLUX_LOWERR_3)mW.m**-2stat.errordoublenullableE_MLFlux3? 1 sigma flux upper error (ML_FLUX_UPERR_3)mW.m**-2stat.error;stat.maxdoublenullableMLBkg3Background flux at the source position (ML_BKG_3)arcmin**-2instr.backgrounddoubleMLExp3Vignetted exposure value in band 3 (ML_EXP_3)sinstr.bandpass;obs.exposuredoubles_MLCtss? 1 sigma counts error; 0.5-2keV (ML_CTS_ERR_s)ctstat.error;phot.countdoublenullables_MLCtst? 1 sigma counts error; 2.3-5keV (ML_CTS_ERR_t)ctstat.error;phot.countdoublenullablee_MLCtst? 1 sigma lower error of counts; 2.3-5keV (ML_CTS_LOWERR_t)ctstat.errordoublenullableE_MLCtst? 1 sigma upper error of counts; 2.3-5keV (ML_CTS_UPERR_t)ctstat.error;stat.maxdoublenullableMLBkgbtBackground flux at the source position; 2.3-5keV (ML_BKG_t)arcmin**-2instr.backgrounddoubleMLExptVignetted exposure value; 2.3-5keV (ML_EXP_t)sstat.value;obs.exposuredoubleMLRatetSource count rate measured by forced PSF-fitting; 2.3-5keV (ML_RATE_t)ct/sphot.count;em.X-raydoubles_MLRatet? 1 sigma count rate error; 2.3-5keV (ML_RATE_ERR_t)ct/sarith.rate;phot.countdoublenullablee_MLRatet? 1 sigma lower error of count rate; 2.3-5keV (ML_RATE_LOWERR_t)ct/sstat.errordoublenullableE_MLRatet? 1 sigma upper error of count rate; 2.3-5keV (ML_RATE_UPERR_t)ct/sstat.error;stat.maxdoublenullableMLEEFtEnclosed energy fraction in the fitting aperture for band h PSF (ML_EEF_t)instr.det.psfdoubleFluxObsMedb2Observed flux in 0.5-1keV, median (FluxObsv_Med_b2)mW.m**-2phot.flux;em.X-raydoublebFluxObsMedb2Observed flux in 0.5-1keV, 1 sigma lower limit (FluxObsv_Lo1_b2)mW.m**-2stat.errordoubleBFluxObsMedb2Observed flux in 0.5-1keV, 1 sigma upper limit (FluxObsv_Up1_b2)mW.m**-2stat.errordoubleb2FluxObsMedb2Observed flux in 0.5-1keV, 2 sigma lower limit (FluxObsv_Lo2_b2)mW.m**-2stat.errordoubleB2FluxObsMedb2Observed flux in 0.5-1keV, 2 sigma upper limit (FluxObsv_Up2_b2)mW.m**-2stat.errordoubleFluxObsMedb3Observed flux in 1-2keV, median (FluxObsv_Med_b3)mW.m**-2phot.flux;em.X-raydoublebFluxObsMedb3Observed flux in 1-2keV, 1 sigma lower limit (FluxObsv_Lo1_b3)mW.m**-2stat.errordoubleBFluxObsMedb3Observed flux in 1-2keV, 1 sigma upper limit (FluxObsv_Up1_b3)mW.m**-2stat.errordoubleb2FluxObsMedb3Observed flux in 1-2keV, 2 sigma lower limit (FluxObsv_Lo2_b3)mW.m**-2stat.errordoubleB2FluxObsMedb3Observed flux in 1-2keV, 2 sigma upper limit (FluxObsv_Up2_b3)mW.m**-2stat.errordoubleFluxObsMedb4Observed flux in 2-4.5keV, median (FluxObsv_Med_b4)mW.m**-2phot.flux;em.X-raydoublebFluxObsMedb4Observed flux in 2-4.5keV, 1 sigma lower limit (FluxObsv_Lo1_b4)mW.m**-2stat.errordoubleBFluxObsMedb4Observed flux in 2-4.5keV, 1 sigma upper limit (FluxObsv_Up1_b4)mW.m**-2stat.errordoubleb2FluxObsMedb4Observed flux in 2-4.5keV, 2 sigma lower limit (FluxObsv_Lo2_b4)mW.m**-2stat.errordoubleB2FluxObsMedb4Observed flux in 2-4.5keV, 2 sigma upper limit (FluxObsv_Up2_b4)mW.m**-2stat.errordoubleExpUnvignetted exposure time (Exp)stime.duration;obs.exposuredoublegalNHIHI column density from HI4PI (galNHI)cm**-2phys.columnDensitydoublegalNHTotal Galactic absorption column density (galNH)cm**-2physdoubleECF-0d2-0d6Energy conversion factor between ML_FLUX_1 and ML_RATE_1 (in cm^2^/erg) (ECF_0d2_0d6)1e+07cm**2.J**-1instr.paramdoubleECF-0.6-2.3Energy conversion factor between ML_FLUX_2 and ML_RATE_2 (in cm^2^/erg) (ECF_0d6_2d3)1e+07cm**2.J**-1instr.paramdoubleECF-2.3-5Energy conversion factor between ML_FLUX_3 and ML_RATE_3 (in cm^2^/erg) (ECF_2d3_5)1e+07cm**2.J**-1instr.paramdoubleMLEEF3Enclosed energy fraction in the fitting aperture for band 3 PSF (ML_EEF_3)instr.det.psfdoubleMLCtssSource net counts measured from count rate; 0.5-2keV (ML_CTS_s)ctphot.countdoublee_MLCtss? 1 sigma lower error of counts; 0.5-2keV (ML_CTS_LOWERR_s)ctstat.errordoublenullableE_MLCtss? 1 sigma upper error of counts; 0.5-2keV (ML_CTS_UPERR_s)ctstat.error;stat.maxdoublenullableMLBkgbsBackground flux at the source position; 0.5-2keV (ML_BKG_s)arcmin**-2instr.backgrounddoubleMLExpsVignetted exposure value; 0.5-2keV (ML_EXP_s)sstat.value;obs.exposuredoubleMLRatesSource count rate measured by forced PSF-fitting; 0.5-2keV (ML_RATE_s)ct/sphot.count;em.X-raydoubles_MLRates? 1 sigma count rate error; 0.5-2keV (ML_RATE_ERR_s)ct/sarith.rate;phot.countdoublenullablee_MLRates? 1 sigma lower error of count rate; 0.5-2keV (ML_RATE_LOWERR_s)ct/sstat.errordoublenullableE_MLRates? 1 sigma upper error of count rate; 0.5-2keV (ML_RATE_UPERR_s)ct/sstat.error;stat.maxdoublenullableMLEEFsEnclosed energy fraction in the fitting aperture for band s PSF (ML_EEF_s)instr.det.psfdoubleMLFluxsSource flux converted from count rate; 0.5-2keV (ML_FLUX_s)mW.m**-2phot.flux;em.X-raydoubles_MLFluxs? 1 sigma flux error; 0.5-2keV (ML_FLUX_ERR_s)mW.m**-2stat.error;phot.fluxdoublenullablee_MLFluxs? 1 sigma lower error of flux; 0.5-2keV (ML_FLUX_LOWERR_s)mW.m**-2stat.errordoublenullableE_MLFluxs? 1 sigma upper error of flux; 0.5-2keV (ML_FLUX_UPERR_s)mW.m**-2stat.error;stat.maxdoublenullableMLCtstSource net counts measured from count rate; 2.3-5keV (ML_CTS_t)ctphot.countdoubleMLFluxhSource flux converted from count rate; 2-10keV (ML_FLUX_h)mW.m**-2phot.flux;em.X-raydoubles_MLFluxh? 1 sigma flux error; 2-10keV (ML_FLUX_ERR_h)mW.m**-2stat.error;phot.fluxdoublenullablee_MLFluxh? 1 sigma lower error of flux; 2-10keV (ML_FLUX_LOWERR_h)mW.m**-2stat.errordoublenullableE_MLFluxh? 1 sigma upper error of flux; 2-10keV (ML_FLUX_UPERR_h)mW.m**-2stat.error;stat.maxdoublenullableApCtssTotal counts extracted in the aperture; 0.5-2keV (APE_CTS_s)ctphot.count;em.X-rayintApBkgsBackground counts in the aperture, excluding nearby sources; 0.5-2keV (APE_BKG_s)ctphot.count;em.X-raydoubleApExPsVignetted exposure value; 0.5-2keV (APE_EXP_s)sstat.value;obs.exposuredoubleApRadsAperture radius; 0.5-2keV (APE_RADIUS_s)pixstat.fit.paramdoubleApPoissPoisson probability of being background fluctuation; 0.5-2keV (APE_POIS_s)stat.fit.goodnessdoubleApCtstTotal counts extracted in the aperture; 2.3-5keV (APE_CTS_t)ctphot.count;em.X-rayintApBkgbtBackground counts in the aperture, excluding nearby sources; 2.3-5keV (APE_BKG_t)ctinstr.backgrounddoubleApExptVignetted exposure value; 2.3-5keV (APE_EXP_t)sstat.value;obs.exposuredoubleApRadtAperture radius; 2.3-5keV (APE_RADIUS_t)pixstat.fit.paramdoubleApPoistPoisson probability of being background fluctuation; 2.3-5keV (APE_POIS_t)stat.fit.goodnessdoubleFluxObsMedb1Observed flux in 0.2-0.5keV, median (FluxObsv_Med_b1)mW.m**-2phot.flux;em.X-raydoublebFluxObsMedb1Observed flux in 0.2-0.5keV, 1 sigma lower limit (FluxObsv_Lo1_b1)mW.m**-2stat.errordoubleBFluxObsMedb1Observed flux in 0.2-0.5keV, 1 sigma upper limit (FluxObsv_Up1_b1)mW.m**-2stat.errordoubleb2FluxObsMedb1Observed flux in 0.2-0.5keV, 2 sigma lower limit (FluxObsv_Lo2_b1)mW.m**-2stat.errordoubleB2FluxObsMedb1Observed flux in 0.2-0.5keV, 2 sigma upper limit (FluxObsv_Up2_b1)mW.m**-2stat.errordoubleFluxObsMedtObserved flux in 2.3-5keV, median (FluxObsv_Med_t)mW.m**-2phot.flux;em.X-raydoublebFluxObsMedtObserved flux in 2.3-5keV, 1 sigma lower limit (FluxObsv_Lo1_t)mW.m**-2stat.errordoubleBFluxObsMedtObserved flux in 2.3-5keV, 1 sigma upper limit (FluxObsv_Up1_t)mW.m**-2stat.errordoubleb2FluxObsMedtObserved flux in 2.3-5keV, 2 sigma lower limit (FluxObsv_Lo2_t)mW.m**-2stat.errordoubleB2FluxObsMedtObserved flux in 2.3-5keV, 2 sigma upper limit (FluxObsv_Up2_t)mW.m**-2stat.errordoubleJ/A+A/664/A126/calpvctpThe counterparts of the X-ray sources, converted from CalPVexG_CTP_V3.3.fitsUIDUnique source ID (UID)meta.idcharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintFieldField name (Field)meta.id;obs.fieldcharID-SRC[1/2794] Source ID in each field (ID_SRC)meta.idintRAcRight ascension (ICRS), corrected using CatWISE2020 (RA_corr)degpos.eq.ra;meta.mainDEcDeclination (ICRS), corrected using CatWISE2020 (DEC_corr)degpos.eq.dec;meta.mainePosCombined positional error, corrected (RADEC_ERR_corr)arcsecstat.error;posdoubleCW2NameCatWISE source name (CW2_source_name)meta.id;meta.maincharCW2IDCatWISE source ID (CW2_source_id)meta.idcharRAWdegCatWISE right ascension (ICRS) at Ep=2015 (CW2_ra)degpos.eq.raDEWdegCatWISE declination (ICRS) at Ep=2015 (CW2_dec)degpos.eq.dece_RAWdegCatWISE RA error (CW2_sigra)arcsecstat.errorfloate_DEWdegCatWISE DE error (CW2_sigdec)arcsecstat.errorfloatW1magCatWISE W1 magnitude (CW2_w1mag)magphot.mag;em.IR.3-4umfloate_W1mag? CatWISE W1 magnitude error (CW2_w1sigm)magstat.error;phot.magfloatnullableW2magCatWISE W2 magnitude error (CW2_w2mag)magphot.mag;em.IR.4-8umfloate_W2mag? CatWISE W2 magnitude error (CW2_w2sigm)magstat.error;phot.magfloatnullableDistpost[0/1] distance posterior probability (dist_post)stat.fit.goodnessdoublepany[0/1] the probability that any of the associations is the correct one (p_any)stat.fit.goodnessdoublepi[0/1] relative probability of the match (p_i)stat.fit.goodnessdoublepX[0/1] probability of being X-ray source based only on the WISE photometry (p_X)stat.fit.goodnessdoubleMatchFlag[1/2] 1 for the most probable match, 2 for secondary match (match_flag)meta.codeintSepSeparation between the pair of sources in arcsec (Separation)arcsecpos.angDistancedoubleGaiaEDR3? Gaia EDR3 unique source ID (GA_source_id)meta.iddoublenullableRAGdeg? Gaia right ascension (ICRS) at Ep=2016 (GA_ra)degpos.eq.ranullablee_RAGdeg? Gaia RA error (GA_ra_error)masstat.errordoublenullableDEGdeg? Gaia declination (ICRS) at Ep=2016 (GA_dec)degpos.eq.decnullablee_DEGdeg? Gaia DEC error (GA_dec_error)masstat.errordoublenullableplx? Gaia absolute stellar parallax (GA_parallax)maspos.parallax.trigdoublenullablee_plx? Gaia parallax error (GA_parallax_error)masstat.error;pos.parallaxdoublenullablepmRA? Gaia proper motion in RA (pmRA*cosDE) (GA_pmra)mas/yrpos.pm;pos.eq.radoublenullablee_pmRA? Gaia RA proper motion error (GA_pmra_error)mas/yrstat.error;pos.pm;pos.eq.radoublenullablepmDE? Gaia proper motion in DE (GA_pmdec)mas/yrpos.pm;pos.eq.decdoublenullablee_pmDE? Gaia DEC proper motion error (GA_pmdec_error)mas/yrstat.error;pos.pm;pos.eq.decdoublenullableJ/A+A/664/A126/calpvaryA list of variable sources, converted from CalPVexG_vary_V3.3.fitsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintUIDUnique source ID (UID)meta.idcharb_TTime of the low-rate bin (T_lo)stime.epochlongB_TTime of the high-rate bin (T_hi)stime.epochlongb_Rate0.2-5keV count rate of the low-rate bin (Rate_lo)ct/sarith.rate;phot.count;em.X-ray.mediumdoubleB_Rate0.2-5keV count rate of the high-rate bin (Rate_hi)ct/sarith.rate;phot.count;em.X-ray.mediumfloatVVariability amplitude (V)src.var.amplitudefloatSVariability significance (S)stat.fit.goodnessfloatmCtsMinimum counts in each bin (mCts)ctphot.count;em.X-rayint