J/A+A/709/A37/blazecatThe BLAZE catalogrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNameCommon name of the source (SRC_NAME)meta.id;meta.maincharRAJ2000Right ascension (J2000) from input catalog (RAJ2000)degpos.eq.ra;meta.mainindexedDEJ2000Declination (J2000) from input catalog (DECJ2000)degpos.eq.dec;meta.mainindexedGLONGalactic longitude from input catalog (LII)degpos.galactic.lonGLATGalactic latitude from input catalog (BII)degpos.galactic.latdoubleClassClassification given by the input catalog (BLAZAR_CLASS)src.classcharz? Redshift given in the input catalog (Z)src.redshiftdoublenullabler_zReference for the redshift (Z_REF)meta.ref;pos.framecharERO-Exp? eROSITA exposure time at source position, if available (ERO_EXPO)stime.duration;obs.exposuredoublenullableulEROFlux? Upper limit 0.2-2.3keV flux, based on exposure time and sensitivity (ERO_UL_FLUX)mW.m**-2phot.flux;em.X-raydoublenullableulEROLum? Upper limit for the 0.2-2.3keV luminosity band based on ERO_UL_FLUX (ERO_UL_LUM)0.1uWphot.flux;em.X-raydoublenullable
J/A+A/709/A37/blazeunvThe unverified BLAZE catalogNameCommon name of the source (SRC_NAME)meta.id;meta.maincharClassClassification given by the input catalog (BLAZAR_CLASS)src.classcharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintRAJ2000Right ascension (J2000) from input catalog (RAJ2000)degpos.eq.ra;meta.mainDEJ2000Declination (J2000) from input catalog (DECJ2000)degpos.eq.dec;meta.mainGLONGalactic longitude from input catalog (LII)degpos.galactic.lonGLATGalactic latitude from input catalog (BII)degpos.galactic.latdoublez? Redshift given in the input catalog (Z)src.redshiftdoublenullabler_zReference for the redshift (Z_REF)meta.ref;pos.framecharERO-Exp? eROSITA exposure time at source position, if available (ERO_EXPO)stime.duration;obs.exposuredoublenullableulEROFlux? Upper limit 0.2-2.3keV flux, based on exposure time and sensitivity (ERO_UL_FLUX)mW.m**-2phot.flux;em.X-raydoublenullableulEROLum? Upper limit for the 0.2-2.3keV luminosity band based on ERO_UL_FLUX (ERO_UL_LUM)0.1uWphot.flux;em.X-raydoublenullableRemoveFlag[1/5] Remove flag (REMOVE_FLAG) (1)meta.codeint
J/A+A/709/A37/blazer1cThe BlazEr1 catalog (slim version)ConfBlazar[0/1] 1 for confirmed blazars and 0 for candidates (CONF_BLAZAR)meta.codeintFGLsrcNameName of source if listed in 4FGL (4FGL-DR4, Abdollahi et al., 2022, Cat. IX/67) (FGL_SRC_NAME)meta.idcharBZCATsrcNameName of source if listed in BZCAT (Massaro et al. 2015 Cat. VII/274) (BZCAT_SRC_NAME)meta.idcharHSPsrcNameName of source if listed in 3HSP (Chang et al, 2019, Cat. J/A+A/632/A77) (HSP_SRC_NAME)meta.idcharHIGHZsrcNameName of source if listed in the HighZ sample (Sbarrato et al., 2026, arXiv:2603.24659, Marcotulli et al., 2025ApJ...979L...6M) (HIGHZ_SRC_NAME)meta.idcharDECdegDeclination of eROSITA source (DEC)degpos.eq.dece_DECdeg? Lower uncertainty of DEC (e_DEC_ERR)arcsecstat.errordoublenullableE_DECdeg? Upper uncertainty of DEC (E_DEC_ERR)arcsecstat.error;stat.maxdoublenullableRARdegRight ascension of eROSITA source without applying the eROSITA aspect correction (RA_RAW)degpos.eq.raDERdegDeclination of eROSITA source without applying the eROSITA aspect correction (DEC_RAW)degpos.eq.decposErr1sigma position uncertainty (POS_ERR)arcsecstat.error;posdoubleMLctsP1ML source net counts in 0.2-0.5 keV keV band (ML_CTS_P1)ctphot.count;em.X-raydoubleMLExpP2ML vignetted exposure time at the source position in 0.5-1.0 keV band (ML_EXP_P2)stime.duration;obs.exposuredoubleMLEefP2ML enclosed energy fraction in 0.5-1.0 keV band (ML_EEF_P2)phys.energydoubleAPEctsP2Total counts extracted within the aperture in 0.5-1.0 keV band (APE_CTS_P2)ctphot.count;em.X-rayintAPEBkgP2Background counts extracted within the aperture, excluding nearby sources using the source map in 0.5-1.0 keV band (APE_BKG_P2)ctinstr.backgrounddoubleAPEExpP2Exposure map value at the given position in 0.5-1.0 keV band (APE_EXP_P2)stime.expodoubleAPERadP2Extraction radius in 0.5-1.0 keV band (APE_RADIUS_P2)pixphys.angSize;em.X-ray.softdoubleAPEPoisP2? Poisson probability that the extracted counts (APE_CTS) are background fluctuation in 0.5-1.0 keV band (APE_POIS_P2)stat.fit.goodnessdoublenullableAPERadP3Extraction radius in 1.0-2.0 keV band (APE_RADIUS_P3)pixphys.angSize;em.X-ray.softdoubleAPEPoisP3? Poisson probability that the extracted counts (APE_CTS) are background fluctuation in 1.0-2.0 keV band (APE_POIS_P3)stat.fit.goodnessdoublenullableDetLikeP4? Detection likelihood in 2.0-5.0 keV band (DET_LIKE_P4)stat.likelihooddoublenullableMLctsP4ML source net counts in 2.0-5.0 keV band (ML_CTS_P4)ctphot.count;em.X-raydoubles_MLctsP4Uncertainty of ML_CTS_P4 (ML_CTS_P4_ERR)ctstat.errordoublee_MLctsP4Lower uncertainty of MLctsP4 (e_ML_CTS_P4_ASYM_ERR)ctstat.errordoubleE_MLctsP4Upper uncertainty of MLctsP4 (E_ML_CTS_P4_ASYM_ERR)ctstat.error;stat.maxdoubleMLRateP4ML source count rate in 2.0-5.0 keV band (ML_RATE_P4)ct/sphot.count;em.X-raydoubles_MLRateP4Uncertainty of ML_RATE_P4 (ML_RATE_P4_ERR)ct/sstat.errordoublee_MLRateP4Lower uncertainty of MLRateP4 (e_ML_RATE_P4_ASYM_ERR)ct/sstat.errordoubleE_MLRateP4Upper uncertainty of MLRateP4 (E_ML_RATE_P4_ASYM_ERR)ct/sstat.error;stat.maxdoubleMLFluxP4ML source flux in 2.0-5.0 keV band (ML_FLUX_P4)mW.m**-2phot.flux;em.X-raydoubles_MLFluxP4Uncertainty of ML_FLUX_P4 (ML_FLUX_P4_ERR)mW.m**-2stat.errordoublee_MLFluxP4Lower uncertainty of MLFluxP4 (e_ML_FLUX_P4_ASYM_ERR)mW.m**-2stat.errordoubleE_MLFluxP4Upper uncertainty of MLFluxP4 (E_ML_FLUX_P4_ASYM_ERR)mW.m**-2stat.error;stat.maxdoubleMLBkgP4ML background counts at the source position in 2.0-5.0 keV band (ML_BKG_P4)arcmin**-2instr.backgrounddoubleMLExpP4ML vignetted exposure time at the source position in 2.0-5.0 keV band (ML_EXP_P4)stime.duration;obs.exposuredoubleMLEefP4ML enclosed energy fraction in 2.0-5.0 keV band (ML_EEF_P4)phys.energydoubleAPERadP4Extraction radius in 2.0-5.0 keV band (APE_RADIUS_P4)pixphys.angSize;em.X-ray.mediumdoubleAPEPoisP4? Poisson probability that the extracted counts (APE_CTS) are background fluctuation in 2.0-5.0 keV band (APE_POIS_P4)stat.fit.goodnessdoublenullableDetLikeP5? Detection likelihood in 5.0-8.0 keV band (DET_LIKE_P5)stat.likelihooddoublenullableMLctsP5ML source net counts in 5.0-8.0 keV keV band (ML_CTS_P5)ctphot.count;em.X-raydoubles_MLctsP5Uncertainty of ML_CTS_P5 (ML_CTS_P5_ERR)ctstat.errordoubleMLEefP6ML enclosed energy fraction in 4.0-10.0 keV band (ML_EEF_P6)phys.energydoubleMLctsP9ML source net counts in 7.2-8.2 keV keV band (ML_CTS_P9)ctphot.count;em.X-raydoubles_MLctsP9Uncertainty of ML_CTS_P9 (ML_CTS_P9_ERR)ctstat.errordoublee_MLctsP9Lower uncertainty of MLctsP9 (e_ML_CTS_P9_ASYM_ERR)ctstat.errordoubleE_MLctsP9Upper uncertainty of MLctsP9 (E_ML_CTS_P9_ASYM_ERR)ctstat.error;stat.maxdoubleMLRateP9ML source count rate in 7.2-8.2 keV band (ML_RATE_P9)ct/sphot.count;em.X-raydoubles_MLRateP9Uncertainty of ML_RATE_P9 (ML_RATE_P9_ERR)ct/sstat.errordoublee_MLRateP9Lower uncertainty of MLRateP9 (e_ML_RATE_P9_ASYM_ERR)ct/sstat.errordoubleE_MLRateP9Upper uncertainty of MLRateP9 (E_ML_RATE_P9_ASYM_ERR)ct/sstat.error;stat.maxdoubleMLFluxP9ML source flux in 7.2-8.2 keV band (ML_FLUX_P9)mW.m**-2phot.flux;em.X-raydoubles_MLFluxP9Uncertainty of ML_FLUX_P9 (ML_FLUX_P9_ERR)mW.m**-2stat.errordoublee_MLFluxP9Lower uncertainty of MLFluxP9 (e_ML_FLUX_P9_ASYM_ERR)mW.m**-2stat.errordoubleE_MLFluxP9Upper uncertainty of MLFluxP9 (E_ML_FLUX_P9_ASYM_ERR)mW.m**-2stat.error;stat.maxdoubleMLBkgP9ML background counts at the source position in 7.2-8.2 keV band (ML_BKG_P9)arcmin**-2instr.backgrounddoubleMLExpP9ML vignetted exposure time at the source position in 7.2-8.2 keV band (ML_EXP_P9)stime.duration;obs.exposuredoubleMLEefP9ML enclosed energy fraction in 7.2-8.2 keV band (ML_EEF_P9)phys.energydoubleAPEctsP9Total counts extracted within the aperture in 7.2-8.2 keV band (APE_CTS_P9)ctphot.count;em.X-rayintAPERadP9Extraction radius in 7.2-8.2 keV band (APE_RADIUS_P9)pixphys.angSize;em.X-ray.mediumdoubleAPEExpSExposure map value at the given position in 0.5-2.0 keV band (APE_EXP_S)stime.expodoubleAPEPoisSPoisson probability that the extracted counts (APE_CTS) are background fluctuation in 0.5-2.0 keV band (APE_POIS_S)stat.fit.goodnessdoubleFSPSNR[0/1] If 1, source may lie within an overdense region near a supernova remnant (FLAG_SP_SNR)meta.codeintPWL15Norm? Power law norm using a fixed N_H and an index of 1.5 at 1 keV (PWL15_NORM)ph.keV**-1.s**-1.cm**-2stat.fit.paramdoublenullablee_PWL15Norm? Lower uncertainty of PWL15Norm (e_PWL15_NORM_ERR)ph.keV**-1.s**-1.cm**-2stat.errordoublenullableE_PWL15Norm? Upper uncertainty of PWL15Norm (E_PWL15_NORM_ERR)ph.keV**-1.s**-1.cm**-2stat.error;stat.maxdoublenullablePWL17Cvar? Variance of Cash statistics of fixed N_H and fixed power law index 1.7 fit according to Kaastra et al., 2017A&A...605A..51K (PWL17_C_VARIANCE)stat.fit.paramdoublenullablePWL20CStatTh? Theoretical Cash statistics while using a fixed N_H and fixed power law index 2.0 fit according to Kaastra et ai., 2017A&A...605A..51K (PWL20_CSTAT_THEORY)stat.fit.paramdoublenullablePWL20redCash? Reduced Cash statistics from fit with fixed N_H and fixed power law index 2.0 (PWL20_REDCASH)stat.fit.paramdoublenullableFreeGAMMA? Power law photon index using a free N_H (FREE_GAMMA)stat.fit.paramdoublenullablee_FreeGAMMA? Lower uncertainty of FreeGAMMA (e_FREE_GAMMA_ERR)stat.errordoublenullableE_FreeGAMMA? Upper uncertainty of FreeGAMMA (E_FREE_GAMMA_ERR)stat.error;stat.maxdoublenullableFreeNorm? Power law norm using a free N_H at 1 keV (FREE_NORM)ph.keV**-1.s**-1.cm**-2stat.fit.paramdoublenullablee_FreeNorm? Lower uncertainty of FreeNorm (e_FREE_NORM_ERR)ph.keV**-1.s**-1.cm**-2stat.errordoublenullableE_FreeNorm? Upper uncertainty of FreeNorm (E_FREE_NORM_ERR)ph.keV**-1.s**-1.cm**-2stat.error;stat.maxdoublenullableFreeFluxunabs0? Fitted unabsorbed flux for a free N_H power law fit in 0.2-2.3 keV band (FREE_FLUX_UNABS_0)mW.m**-2stat.fit.paramdoublenullablee_FreeFluxunabs0? Lower uncertainty of FreeFluxunabs0 (e_FREE_FLUX_UNABS_0_ERR)mW.m**-2stat.errordoublenullableE_FreeFluxunabs0? Upper uncertainty of FreeFluxunabs0 (E_FREE_FLUX_UNABS_0_ERR)mW.m**-2stat.error;stat.maxdoublenullableFreeFluxabs0? Fitted observed flux for a free N_H power law fit in 0.2-2.3 keV band (FREE_FLUX_ABS_0)mW.m**-2stat.fit.paramdoublenullablee_FreeFluxabs0? Lower uncertainty of FreeFluxabs0 (e_FREE_FLUX_ABS_0_ERR)mW.m**-2stat.errordoublenullableE_FreeFluxabs0? Upper uncertainty of FreeFluxabs0 (E_FREE_FLUX_ABS_0_ERR)mW.m**-2stat.error;stat.maxdoublenullableFreeCvar? Variance of Cash statistics of free N_H power law fit according to Kaastra et ai., 2017A&A...605A..51K (FREE_C_VARIANCE)stat.fit.paramdoublenullableFreeCash? Cash statistics of free N_H power law fit (FREE_CASH)stat.fit.paramdoublenullableFreeCStatTh? Theoretical Cash statistics while using a free N_H power law fit according to Kaastra et ai., 2017A&A...605A..51K (FREE_CSTAT_THEORY)stat.fit.paramdoublenullableFreeredCash? Reduced Cash statistics from fit with free N_H (FREE_REDCASH)stat.fit.paramdoublenullableFreeCashBinsNumber of bins used during the free N_H power law fit (FREE_CASHBINS)stat.fit.paramFreeCashParNumber of parameters used during the free N_H power law fit (FREE_CASHPAR)stat.fit.paramFreeNumBinsNumber of bins used to calculate Kaastra et ai., 2017A&A...605A..51K values of free N_H power law fit (FREE_NUM_BINS)stat.fit.paramFixedNH? Fixed N_H (FIXED_NH)cm**-2stat.fit.paramdoublenullableFixedGAMMA? Power law photon index using a fixed N_H (FIXED_GAMMA)stat.fit.paramdoublenullablee_FixedGAMMA? Lower uncertainty of Fixed_GAMMA (e_FIXED_GAMMA_ERR)stat.errordoublenullableE_FixedGAMMA? Upper uncertainty of Fixed_GAMMA (E_FIXED_GAMMA_ERR)stat.error;stat.maxdoublenullableFixedNorm? Power law norm using a fixed N_H at 1 keV (FIXED_NORM)ph.keV**-1.s**-1.cm**-2stat.fit.paramdoublenullablee_FixedNorm? Lower uncertainty of FixedNorm (e_FIXED_NORM_ERR)ph.keV**-1.s**-1.cm**-2stat.errordoublenullableE_FixedNorm? Upper uncertainty of FixedNorm (E_FIXED_NORM_ERR)ph.keV**-1.s**-1.cm**-2stat.error;stat.maxdoublenullableFixedFluxunabs0? Fitted unabsorbed flux for a fixed N_H power law fit in 0.2-2.3 keV band (FIXED_FLUX_UNABS_0)mW.m**-2stat.fit.paramdoublenullablee_FixedFluxunabs0? Lower uncertainty of FixedFluxunabs0 (e_FIXED_FLUX_UNABS_0_ERR)mW.m**-2stat.errordoublenullableE_FixedFluxunabs0? Upper uncertainty of FixedFluxunabs0 (E_FIXED_FLUX_UNABS_0_ERR)mW.m**-2stat.error;stat.maxdoublenullableFixedFluxabs0? Fitted observed flux for a fixed N_H power law fit in 0.2-2.3 keV band (FIXED_FLUX_ABS_0)mW.m**-2stat.fit.paramdoublenullablee_FixedFluxabs0? Lower uncertainty of FixedFluxabs0 (e_FIXED_FLUX_ABS_0_ERR)mW.m**-2stat.errordoublenullableE_FixedFluxabs0? Upper uncertainty of FixedFluxabs0 (E_FIXED_FLUX_ABS_0_ERR)mW.m**-2stat.error;stat.maxdoublenullableFixedCvar? Variance of Cash statistics of fixed N_H power law fit according to Kaastra et ai., 2017A&A...605A..51K (FIXED_C_VARIANCE)stat.fit.paramdoublenullableFixedCash? Cash statistics of fixed N_H power law fit (FIXED_CASH)stat.fit.paramdoublenullableFixedCStatTh? Theoretical Cash statistics while using a fixed N_H power law fit according to Kaastra et ai., 2017A&A...605A..51K (FIXED_CSTAT_THEORY)stat.fit.paramdoublenullableFixedredCash? Reduced Cash statistics from fit with fixed N_H (FIXED_REDCASH)stat.fit.paramdoublenullableFixedCashBinsNumber of bins used during the fixed N_H power law fit (FIXED_CASHBINS)stat.fit.paramFixedCashParNumber of parameters used during the fixed N_H power law fit (FIXED_CASHPAR)stat.fit.paramrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNameCommon name of the source (SRC_NAME)meta.id;meta.maincharRAJ2000Right ascension (J2000) from input catalog (RAJ2000)degpos.eq.ra;meta.mainDEJ2000Declination (J2000) from input catalog (DECJ2000)degpos.eq.dec;meta.mainClassBlazar classification given by the input catalog (BLAZAR_CLASS)src.classcharMILLIQUASsrcNameName of source if listed in Milliquas (Flesch et al., 2023, Cat. Cat. V/158) (MILLIQUAS_SRC_NAME)meta.idcharKDEBLLACSsrcNameName of source if listed in KDEBLLACS (Dabrusco et al., 2019, Cat. J/ApJS/242/4) (KDEBLLACS_SRC_NAME)meta.idcharWIBRALS2srcNameName of source if listed in WIBRaLS2 (Dabrusco et al., 2019, Cat. J/ApJS/242/4) (WIBRALS2_SRC_NAME)meta.idcharABCsrcNameName of source if listed in ABC (Paggi et al., 2020, Cat. J/A+A/641/A62) (ABC_SRC_NAME)meta.idcharBROSsrcNameName of source if listed in BROS (Itoh et al., 2020, Cat. J/ApJ/901/3) (BROS_SRC_NAME)meta.idcharSepAngular separation between catalog and eROSITA position (ANGSEP)degpos.angDistancedoubleDetUIdeROSITA unique detection ID (DETUID)meta.idcharIAUNameOfficial IAU name of the eROSITA source, 1eRASS JHHMMSS.s+DDMMSS (IAUNAME)meta.idcharSkyTileeROSITA sky tile ID (SKYTILE)obs.fieldintIdSrceROSITA source ID in each sky tile (ID_SRC)meta.idintUIdInteger unique detection ID. See Merloni et al., 2024, Cat. J/A+A/682/A34 for details (UID)meta.idUIdHardHard catalog UID of the source with a strong association, or -UID if the association is weak. 0 means no counterpart found in the Hard catalog (UID_HARD)meta.idIdClusterGroup ID of sources simultaneously modeled during source detection (ID_CLUSTER)meta.id.parentintRACdegRight ascension of eROSITA source (RA)degpos.eq.rae_RACdeg? Lower uncertainty of RA (e_RA_ERR)arcsecstat.errordoublenullableE_RACdeg? Upper uncertainty of RA (E_RA_ERR)arcsecstat.error;stat.maxdoublenullableRADEErrCombined positional error, raw output from PSF fitting (RADEC_ERR)arcsecstat.error;posGLONGalactic longitude of eROSITA source with applied position correction (not identical to the coordinates listed by Merloni+2024) (LII)degpos.galactic.lonGLATGalactic latitude of eROSITA source with applied position correction (not identical to the coordinates listed by Merloni+2024) (BII)degpos.galactic.latdoubleELONEquatorial longitude of eROSITA source (ELON)degpos.ecliptic.lonELATEquatorial latitude of eROSITA source (ELAT)degpos.ecliptic.latdoubleMJDModified Julian Date of the observation of the source nearest to the optical axis of eROSITA (MJD)dtime.epochdoubleb_MJDModified Julian Date of the sources' first eROSITA observation (MJD_MIN)dtime.epochdoubleB_MJDModified Julian Date of the sources' last eROSITA observation (MJD_MAX)dtime.epochdoubleDetLike0Detection likelihood in 0.2-2.3 keV band (DET_LIKE_0)stat.likelihooddoubleMLcts1? ML source net counts in 0.2-2.3 keV band (ML_CTS_1)ctphot.count;em.X-raydoublenullables_MLcts1? Uncertainty of MLcts1 (ML_CTS_1_ERR)ctstat.errordoublenullablee_MLcts1? Lower uncertainty of MLcts1 (e_ML_CTS_1_ASYM_ERR)ctstat.errordoublenullableE_MLcts1? Upper uncertainty of MLcts1 (E_ML_CTS_1_ASYM_ERR)ctstat.error;stat.maxdoublenullableMLRate1? ML source count rate in 0.2-2.3 keV band (ML_RATE_1)ct/sphot.count;em.X-raydoublenullables_MLRate1? Uncertainty of MLRate1 (ML_RATE_1_ERR)ct/sstat.errordoublenullablee_s_MLRate1? Lower uncertainty of MLRate1 (e_MLRate1_ASYM_ERR)ct/sstat.errordoublenullableE_s_MLRate1? Upper uncertainty of MLRate1 (E_ML_RATE_1_ASYM_ERR)ct/sstat.error;stat.maxdoublenullableMLFlux1ML source flux in 0.2-2.3 keV band (ML_FLUX_1)mW.m**-2phot.flux;em.X-raydoubles_MLFlux1? Uncertainty of MLFlux1 (ML_FLUX_1_ERR)mW.m**-2stat.errordoublenullablee_MLFlux1? Lower uncertainty of MLFlux1 (e_ML_FLUX_1_ASYM_ERR)mW.m**-2stat.errordoublenullableE_MLFlux1? Upper uncertainty of MLFlux1 (E_ML_FLUX_1_ASYM_ERR)mW.m**-2stat.error;stat.maxdoublenullableMLBkg1ML background counts at the source position in 0.2-2.3 keV band (ML_BKG_1)arcmin**-2instr.backgrounddoubleMLExp1ML vignetted exposure time at the source position in 0.2-2.3 keV band (ML_EXP_1)stime.duration;obs.exposuredoubleMLEef1ML enclosed energy fraction in 0.2-2.3 keV band (ML_EEF_1)phys.energydoubleAPEcts1Total counts extracted within the aperture in 0.2-2.3 keV band (APE_CTS_1)ctphot.count;em.X-rayintAPEBkg1Background counts extracted within the aperture, excluding nearby sources using the source map in 0.2-2.3 keV band (APE_BKG_1)ctinstr.backgrounddoubleAPEExp1Exposure map value at the given position in 0.2-2.3 keV band (APE_EXP_1)stime.expodoubleAPERad1Extraction radius in 0.2-2.3 keV band (APE_RADIUS_1)pixphys.angSize;em.X-ray.softdoubleAPEPois1? Poisson probability that the extracted counts (APE_CTS) are background fluctuation in 0.2-2.3 keV band (APE_POIS_1)stat.fit.goodnessdoublenullableDetLikeP1? Detection likelihood in 0.2-0.5 keV band (DET_LIKE_P1)stat.likelihooddoublenullables_MLctsP1Uncertainty of MLctsP1 (ML_CTS_P1_ERR)ctstat.errordoublee_MLctsP1Lower uncertainty of MLctsP1 (e_ML_CTS_P1_ASYM_ERR)ctstat.errordoubleE_MLctsP1Upper uncertainty of MLctsP1 (E_ML_CTS_P1_ASYM_ERR)ctstat.error;stat.maxdoubleMLRateP1ML source count rate in 0.2-0.5 keV band (ML_RATE_P1)ct/sphot.count;em.X-raydoubles_MLRateP1Uncertainty of MLRateP1 (ML_RATE_P1_ERR)ct/sstat.errordoublee_MLRateP1Lower uncertainty of MLRateP1 (e_MLRateP1_ASYM_ERR)ct/sstat.errordoubleE_MLRateP1Upper uncertainty of MLRateP1 (E_ML_RATE_P1_ASYM_ERR)ct/sstat.error;stat.maxdoubleMLFluxP1ML source flux in 0.2-0.5 keV band (ML_FLUX_P1)mW.m**-2phot.flux;em.X-raydoubles_MLFluxP1Uncertainty of MLFluxP1 (ML_FLUX_P1_ERR)mW.m**-2stat.errordoublee_MLFluxP1Lower uncertainty of MLFluxP1 (e_ML_FLUX_P1_ASYM_ERR)mW.m**-2stat.errordoubleE_MLFluxP1Upper uncertainty of MLFluxP1 (E_ML_FLUX_P1_ASYM_ERR)mW.m**-2stat.error;stat.maxdoubleMLBkgP1ML background counts at the source position in 0.2-0.5 keV band (ML_BKG_P1)arcmin**-2instr.backgrounddoubleMLExpP1ML vignetted exposure time at the source position in 0.2-0.5 keV band (ML_EXP_P1)stime.duration;obs.exposuredoubleMLEefP1ML enclosed energy fraction in 0.2-0.5 keV band (ML_EEF_P1)phys.energydoubleAPEctsP1Total counts extracted within the aperture in 0.2-0.5 keV band (APE_CTS_P1)ctphot.count;em.X-rayintAPEBkgP1Background counts extracted within the aperture, excluding nearby sources using the source map in 0.2-0.5 keV band (APE_BKG_P1)ctinstr.backgrounddoubleAPEExpP1Exposure map value at the given position in 0.2-0.5 keV band (APE_EXP_P1)stime.expodoubleAPERadP1Extraction radius in 0.2-0.5 keV band (APE_RADIUS_P1)pixphys.angSize;em.X-ray.softdoubleAPEPoisP1? Poisson probability that the extracted counts (APE_CTS) are background fluctuation in 0.2-0.5 keV band (APE_POIS_P1)stat.fit.goodnessdoublenullableDetLikeP2Detection likelihood in 0.5-1.0 keV band (DET_LIKE_P2)stat.likelihooddoubleMLctsP2ML source net counts in 0.5-1.0 keV keV band (ML_CTS_P2)ctphot.count;em.X-raydoubles_MLctsP2Uncertainty of MLctsP2 (ML_CTS_P2_ERR)ctstat.errordoublee_MLctsP2Lower uncertainty of MLctsP2 (e_ML_CTS_P2_ASYM_ERR)ctstat.errordoubleE_MLctsP2Upper uncertainty of MLctsP2 (E_ML_CTS_P2_ASYM_ERR)ctstat.error;stat.maxdoubleMLRateP2ML source count rate in 0.5-1.0 keV band (ML_RATE_P2)ct/sphot.count;em.X-raydoubles_MLRateP2Uncertainty of MLRateP2 (ML_RATE_P2_ERR)ct/sstat.errordoublee_MLRateP2Lower uncertainty of MLRateP2 (e_MLRateP2_ASYM_ERR)ct/sstat.errordoubleE_MLRateP2Upper uncertainty of MLRateP2 (E_ML_RATE_P2_ASYM_ERR)ct/sstat.error;stat.maxdoubleMLFluxP2ML source flux in 0.5-1.0 keV keV band (ML_FLUX_P2)mW.m**-2phot.flux;em.X-raydoubles_MLFluxP2Uncertainty of MLFluxP2 (ML_FLUX_P2_ERR)mW.m**-2stat.errordoublee_MLFluxP2Lower uncertainty of MLFluxP2 (e_ML_FLUX_P2_ASYM_ERR)mW.m**-2stat.errordoubleE_MLFluxP2Upper uncertainty of MLFluxP2 (E_ML_FLUX_P2_ASYM_ERR)mW.m**-2stat.error;stat.maxdoubleMLBkgP2ML background counts at the source position in 0.5-1.0 keV band (ML_BKG_P2)arcmin**-2instr.backgrounddoubleDetLikeP3Detection likelihood in 1.0-2.0 keV band (DET_LIKE_P3)stat.likelihooddoubleMLctsP3ML source net counts in 1.0-2.0 keV keV band (ML_CTS_P3)ctphot.count;em.X-raydoubles_MLctsP3Uncertainty of MLctsP3 (ML_CTS_P3_ERR)ctstat.errordoublee_MLctsP3Lower uncertainty of MLctsP3 (e_ML_CTS_P3_ASYM_ERR)ctstat.errordoubleE_MLctsP3Upper uncertainty of MLctsP3 (E_ML_CTS_P3_ASYM_ERR)ctstat.error;stat.maxdoubleMLRateP3ML source count rate in 1.0-2.0 keV band (ML_RATE_P3)ct/sphot.count;em.X-raydoubles_MLRateP3Uncertainty of MLRateP3 (ML_RATE_P3_ERR)ct/sstat.errordoublee_MLRateP3Lower uncertainty of MLRateP3 (e_MLRateP3_ASYM_ERR)ct/sstat.errordoubleE_MLRateP3Upper uncertainty of MLRateP3 (E_ML_RATE_P3_ASYM_ERR)ct/sstat.error;stat.maxdoubleMLFluxP3ML source flux in 1.0-2.0 keV band (ML_FLUX_P3)mW.m**-2phot.flux;em.X-raydoubles_MLFluxP3Uncertainty of MLFluxP3 (ML_FLUX_P3_ERR)mW.m**-2stat.errordoublee_MLFluxP3Lower uncertainty of MLFluxP3 (e_ML_FLUX_P3_ASYM_ERR)mW.m**-2stat.errordoubleE_MLFluxP3Upper uncertainty of MLFluxP3 (E_ML_FLUX_P3_ASYM_ERR)mW.m**-2stat.error;stat.maxdoubleMLBkgP3ML background counts at the source position in 1.0-2.0 keV band (ML_BKG_P3)arcmin**-2instr.backgrounddoubleMLExpP3ML vignetted exposure time at the source position in 1.0-2.0 keV band (ML_EXP_P3)stime.duration;obs.exposuredoubleMLEefP3ML enclosed energy fraction in 1.0-2.0 keV band (ML_EEF_P3)phys.energydoubleAPEctsP3Total counts extracted within the aperture in 1.0-2.0 keV band (APE_CTS_P3)ctphot.count;em.X-rayintAPEBkgP3Background counts extracted within the aperture, excluding nearby sources using the source map in 1.0-2.0 keV band (APE_BKG_P3)ctinstr.backgrounddoubleAPEExpP3Exposure map value at the given position in 1.0-2.0 keV band (APE_EXP_P3)stime.expodoubleAPEctsP4Total counts extracted within the aperture in 2.0-5.0 keV band (APE_CTS_P4)ctphot.count;em.X-rayintAPEBkgP4Background counts extracted within the aperture, excluding nearby sources using the source map in 2.0-5.0 keV band (APE_BKG_P4)ctinstr.backgrounddoubleAPEExpP4Exposure map value at the given position in 2.0-5.0 keV band (APE_EXP_P4)stime.expodoublee_MLctsP5Lower uncertainty of MLctsP5 (e_ML_CTS_P5_ASYM_ERR)ctstat.errordoubleE_MLctsP5Upper uncertainty of MLctsP5 (E_ML_CTS_P5_ASYM_ERR)ctstat.error;stat.maxdoubleMLRateP5ML source count rate in 5.0-8.0 keV band (ML_RATE_P5)ct/sphot.count;em.X-raydoubles_MLRateP5Uncertainty of ML_RATE_P5 (ML_RATE_P5_ERR)ct/sstat.errordoublee_MLRateP5Lower uncertainty of MLRateP5 (e_ML_RATE_P5_ASYM_ERR)ct/sstat.errordoubleE_MLRateP5Upper uncertainty of MLRateP5 (E_ML_RATE_P5_ASYM_ERR)ct/sstat.error;stat.maxdoubles_MLFluxP5ML source flux in 5.0-8.0 keV band (ML_FLUX_P5)mW.m**-2phot.flux;em.X-ray.mediumdoubleMLFluxP5Uncertainty of ML_FLUX_P5 (ML_FLUX_P5_ERR)mW.m**-2phot.flux;em.X-raydoublee_MLFluxP5Lower uncertainty of MLFluxP5 (e_ML_FLUX_P5_ASYM_ERR)mW.m**-2stat.errordoubleE_MLFluxP5Upper uncertainty of MLFluxP5 (E_ML_FLUX_P5_ASYM_ERR)mW.m**-2stat.error;stat.maxdoubleMLBkgP5ML background counts at the source position in 5.0-8.0 keV band (ML_BKG_P5)arcmin**-2instr.backgrounddoubleMLExpP5ML vignetted exposure time at the source position in 5.0-8.0 keV band (ML_EXP_P5)stime.duration;obs.exposuredoubleMLEefP5ML enclosed energy fraction in 5.0-8.0 keV band (ML_EEF_P5)phys.energydoubleAPEctsP5Total counts extracted within the aperture in 5.0-8.0 keV band (APE_CTS_P5)ctphot.count;em.X-rayintAPEBkgP5Background counts extracted within the aperture, excluding nearby sources using the source map in 5.0-8.0 keV band (APE_BKG_P5)ctinstr.backgrounddoubleAPEExpP5Exposure map value at the given position in 5.0-8.0 keV band (APE_EXP_P5)stime.expodoubleAPERadP5Extraction radius in 5.0-8.0 keV band (APE_RADIUS_P5)pixphys.angSize;em.X-ray.mediumdoubleAPEPoisP5? Poisson probability that the extracted counts (APE_CTS) are background fluctuation in 5.0-8.0 keV band (APE_POIS_P5)stat.fit.goodnessdoublenullableDetLikeP6? Detection likelihood in 4.0-10.0 keV band (DET_LIKE_P6)stat.likelihooddoublenullableMLctsP6ML source net counts in 4.0-10.0 keV keV band (ML_CTS_P6)ctphot.count;em.X-raydoubles_MLctsP6Uncertainty of ML_CTS_P6 (ML_CTS_P6_ERR)ctstat.errordoublee_MLctsP6Lower uncertainty of MLctsP6 (e_ML_CTS_P6_ASYM_ERR)ctstat.errordoubleE_MLctsP6Upper uncertainty of MLctsP6 (E_ML_CTS_P6_ASYM_ERR)ctstat.error;stat.maxdoubleMLRateP6ML source count rate in 4.0-10.0 keV band (ML_RATE_P6)ct/sphot.count;em.X-raydoubles_MLRateP6Uncertainty of ML_RATE_P6 (ML_RATE_P6_ERR)ct/sstat.errordoublee_MLRateP6Lower uncertainty of MLRateP6 (e_ML_RATE_P6_ASYM_ERR)ct/sstat.errordoubleE_MLRateP6Upper uncertainty of MLRateP6 (E_ML_RATE_P6_ASYM_ERR)ct/sstat.error;stat.maxdoubleMLFluxP6ML source flux in 4.0-10.0 keV band (ML_FLUX_P6)mW.m**-2phot.flux;em.X-raydoubles_MLFluxP6Uncertainty of ML_FLUX_P6 (ML_FLUX_P6_ERR)mW.m**-2stat.errordoublee_MLFluxP6Lower uncertainty of MLFluxP6 (e_ML_FLUX_P6_ASYM_ERR)mW.m**-2stat.errordoubleE_MLFluxP6Upper uncertainty of MLFluxP6 (E_ML_FLUX_P6_ASYM_ERR)mW.m**-2stat.error;stat.maxdoubleMLBkgP6ML background counts at the source position in 4.0-10.0 keV band (ML_BKG_P6)arcmin**-2instr.backgrounddoubleMLExpP6ML vignetted exposure time at the source position in 4.0-10.0 keV band (ML_EXP_P6)stime.duration;obs.exposuredoubleAPEctsP6Total counts extracted within the aperture in 4.0-10.0 keV band (APE_CTS_P6)ctphot.count;em.X-rayintAPEBkgP6Background counts extracted within the aperture, excluding nearby sources using the source map in 4.0-10.0 keV band (APE_BKG_P6)ctinstr.backgrounddoubleAPEExpP6Exposure map value at the given position in 4.0-10.0 keV band (APE_EXP_P6)stime.expodoubleAPERadP6Extraction radius in 4.0-10.0 keV band (APE_RADIUS_P6)pixphys.angSize;em.X-ray.mediumdoubleAPEPoisP6? Poisson probability that the extracted counts (APE_CTS) are background fluctuation in 4.0-10.0 keV band (APE_POIS_P6)stat.fit.goodnessdoublenullableDetLikeP7? Detection likelihood in 5.1-6.1 keV band (DET_LIKE_P7)stat.likelihooddoublenullableMLctsP7ML source net counts in 5.1-6.1 keV band (ML_CTS_P7)ctphot.count;em.X-raydoubles_MLctsP7Uncertainty of ML_CTS_P7 (ML_CTS_P7_ERR)ctstat.errordoublee_MLctsP7Lower uncertainty of MLctsP7 (e_ML_CTS_P7_ASYM_ERR)ctstat.errordoubleE_MLctsP7Upper uncertainty of MLctsP7 (E_ML_CTS_P7_ASYM_ERR)ctstat.error;stat.maxdoubleMLRateP7ML source count rate in 5.1-6.1 keV band (ML_RATE_P7)ct/sphot.count;em.X-raydoubles_MLRateP7Uncertainty of ML_RATE_P7 (ML_RATE_P7_ERR)ct/sstat.errordoublee_MLRateP7Lower uncertainty of MLRateP7 (e_ML_RATE_P7_ASYM_ERR)ct/sstat.errordoubleE_MLRateP7Upper uncertainty of MLRateP7 (E_ML_RATE_P7_ASYM_ERR)ct/sstat.error;stat.maxdoubleMLFluxP7ML source flux in 5.1-6.1 keV band (ML_FLUX_P7)mW.m**-2phot.flux;em.X-raydoubles_MLFluxP7Uncertainty of ML_FLUX_P7 (ML_FLUX_P7_ERR)mW.m**-2stat.errordoublee_MLFluxP7Lower uncertainty of MLFluxP7 (e_ML_FLUX_P7_ASYM_ERR)mW.m**-2stat.errordoubleE_MLFluxP7Upper uncertainty of MLFluxP7 (E_ML_FLUX_P7_ASYM_ERR)mW.m**-2stat.error;stat.maxdoubleMLBkgP7ML background counts at the source position in 5.1-6.1 keV band (ML_BKG_P7)arcmin**-2instr.backgrounddoubleMLExpP7ML vignetted exposure time at the source position in 5.1-6.1 keV band (ML_EXP_P7)stime.duration;obs.exposuredoubleMLEefP7ML enclosed energy fraction in 5.1-6.1 keV band (ML_EEF_P7)phys.energydoubleAPEctsP7Total counts extracted within the aperture in 5.1-6.1 keV band (APE_CTS_P7)ctphot.count;em.X-rayintAPEBkgP7Background counts extracted within the aperture, excluding nearby sources using the source map in 5.1-6.1 keV band (APE_BKG_P7)ctinstr.backgrounddoubleAPEExpP7Exposure map value at the given position in 5.1-6.1 keV band (APE_EXP_P7)stime.expodoubleAPERadP7Extraction radius in 5.1-6.1 keV band (APE_RADIUS_P7)pixphys.angSize;em.X-ray.mediumdoubleAPEPoisP7? Poisson probability that the extracted counts (APE_CTS) are background fluctuation in 5.1-6.1 keV band (APE_POIS_P7)stat.fit.goodnessdoublenullableDetLikeP8? Detection likelihood in 6.2-7.1 keV band (DET_LIKE_P8)stat.likelihooddoublenullableMLctsP8ML source net counts in 6.2-7.1 keV keV band (ML_CTS_P8)ctphot.count;em.X-raydoubles_MLctsP8Uncertainty of ML_CTS_P8 (ML_CTS_P8_ERR)ctstat.errordoublee_MLctsP8Lower uncertainty of MLctsP8 (e_ML_CTS_P8_ASYM_ERR)ctstat.errordoubleE_MLctsP8Upper uncertainty of MLctsP8 (E_ML_CTS_P8_ASYM_ERR)ctstat.error;stat.maxdoubles_MLRateP8ML source count rate in 6.2-7.1 keV band (ML_RATE_P8)ct/sarith.rate;phot.count;em.X-ray.mediumdoubleMLRateP8Uncertainty of ML_RATE_P8 (ML_RATE_P8_ERR)ct/sphot.count;em.X-raydoublee_MLRateP8Lower uncertainty of MLRateP8 (e_ML_RATE_P8_ASYM_ERR)ct/sstat.errordoubleE_MLRateP8Upper uncertainty of MLRateP8 (E_ML_RATE_P8_ASYM_ERR)ct/sstat.error;stat.maxdoubleMLFluxP8ML source flux in 6.2-7.1 keV band (ML_FLUX_P8)mW.m**-2phot.flux;em.X-raydoubles_MLFluxP8Uncertainty of ML_FLUX_P8 (ML_FLUX_P8_ERR)mW.m**-2stat.errordoublee_MLFluxP8Lower uncertainty of MLFluxP8 (e_ML_FLUX_P8_ASYM_ERR)mW.m**-2stat.errordoubleE_MLFluxP8Upper uncertainty of MLFluxP8 (E_ML_FLUX_P8_ASYM_ERR)mW.m**-2stat.error;stat.maxdoubleMLBkgP8ML background counts at the source position in 6.2-7.1 keV band (ML_BKG_P8)arcmin**-2instr.backgrounddoubleMLExpP8ML vignetted exposure time at the source position in 6.2-7.1 keV band (ML_EXP_P8)stime.duration;obs.exposuredoubleMLEefP8ML enclosed energy fraction in 6.2-7.1 keV band (ML_EEF_P8)phys.energydoubleAPEctsP8Total counts extracted within the aperture in 6.2-7.1 keV band (APE_CTS_P8)ctphot.count;em.X-rayintAPEBkgP8Background counts extracted within the aperture, excluding nearby sources using the source map in 6.2-7.1 keV band (APE_BKG_P8)ctinstr.backgrounddoubleAPEExpP8Exposure map value at the given position in 6.2-7.1 keV band (APE_EXP_P8)stime.expodoubleAPERadP8Extraction radius in 6.2-7.1 keV band (APE_RADIUS_P8)pixphys.angSize;em.X-ray.mediumdoubleAPEPoisP8? Poisson probability that the extracted counts (APE_CTS) are background fluctuation in 6.2-7.1 keV band (APE_POIS_P8)stat.fit.goodnessdoublenullableDetLikeP9? Detection likelihood in 7.2-8.2 keV band (DET_LIKE_P9)stat.likelihooddoublenullableAPEBkgP9Background counts extracted within the aperture, excluding nearby sources using the source map in 7.2-8.2 keV band (APE_BKG_P9)ctinstr.backgrounddoubleAPEExpP9Exposure map value at the given position in 7.2-8.2 keV band (APE_EXP_P9)stime.expodoubleAPEPoisP9? Poisson probability that the extracted counts (APE_CTS) are background fluctuation in 7.2-8.2 keV band (APE_POIS_P9)stat.fit.goodnessdoublenullableAPEctsSTotal counts extracted within the aperture in 0.5-2.0 keV band (APE_CTS_S)ctphot.count;em.X-rayintAPEBkgSBackground counts extracted within the aperture, excluding nearby sources using the source map in 0.5-2.0 keV band (APE_BKG_S)ctinstr.backgrounddoubleFSPBPS[0/1] If 1, source may lie within an overdense region near a bright point source (FLAG_SP_BPS)meta.codeintFSPSCL[0/1] If 1, source may lie within an overdense region near a stellar cluster (FLAG_SP_SCL)meta.codeintFSPLGA[0/1] If 1, source may lie within an overdense region near a local large galaxy (FLAG_SP_LGA)meta.codeintFSPGCCons[0/1] If 1, source may lie within an overdense region near a galaxy cluster (FLAG_SP_GC_CONS)meta.codeintFNORADEerr[0/1] If 1, source contained no RA_DEC in the preprocessed version of the catalog (FLAG_NO_RADEC_ERR)meta.codeintFNOEXTerr[0/1] If 1, source contained no EXT in the preprocessed version of the catalog (FLAG_NO_EXT_ERR)meta.codeintFNOCTSerr[0/1] If 1, source contained no MLcts0 in the preprocessed version of the catalog (FLAG_NO_CTS_ERR)meta.codeintFOPT[0] If 1, source matched with in 15arcsec with a bright optical star, likely contaminated by optical loading (FLAG_OPT)meta.codeintcts1? Counts from spectrum in 0.2-2.3 keV band (CTS_1)ctphot.count;em.X-raydoublenullablee_cts1? Lower uncertainty of cts1 (e_CTS_1_ERR)ctstat.errordoublenullableE_cts1? Upper uncertainty of cts1 (E_CTS_1_ERR)ctstat.error;stat.maxdoublenullablectsT? Counts from spectrum in 0.2-10.0 keV band (CTS_T)ctphot.count;em.X-raydoublenullablee_ctsT? Lower uncertainty of ctsT (e_CTS_T_ERR)ctstat.errordoublenullableE_ctsT? Upper uncertainty of ctsT (E_CTS_T_ERR)ctstat.error;stat.maxdoublenullableSpecExpTime? Exposure time as given in the spectrum (SPEC_EXPOTIME)stime.duration;obs.exposuredoublenullableExpTimeExposure time from the eROSITA exposure map in 0.2-2.3 keV band (EXPOTIME)stime.duration;obs.exposuredoubleMinFlux95Minimum detectable flux at source position to guarantee 95% detection rate with a DetLike0 of 10 or greater in the 0.2-2.3 keV band (MIN_FLUX_95)mW.m**-2phot.flux;em.X-raydoubleAverageNH? Average N_H from the Hi4pi collaboration, 2016, Cat. J/A+A/594/A116 (AVERAGE_NH)cm**-2phys.columnDensitydoublenullableWEAverageNH? Weighted average N_H from the Hi4pi collaboration, 2016, Cat. J/A+A/594/A116 (WE_AVERAGE_NH)cm**-2phys.columnDensitydoublenullableHR12? Hardness ratio between 0.2-0.7 keV and 0.7-1.2 keV (HR12)phot.flux;arith.ratiodoublenullablee_HR12? Lower uncertainty of HR12 (e_HR12_ERR)stat.errordoublenullableE_HR12? Upper uncertainty of HR12 (E_HR12_ERR)stat.error;stat.maxdoublenullableHR23? Hardness ratio between 0.7-1.2 keV and 1.2-2.3 keV (HR23)phot.flux;arith.ratiodoublenullablee_HR23? Lower uncertainty of HR23 (e_HR23_ERR)stat.errordoublenullableE_HR23? Upper uncertainty of HR23 (E_HR23_ERR)stat.error;stat.maxdoublenullableHR13? Hardness ratio between 0.2-0.7 keV and 1.2-2.3 keV (HR13)phot.flux;arith.ratiodoublenullablee_HR13? Lower uncertainty of HR13 (e_HR13_ERR)stat.errordoublenullableE_HR13? Upper uncertainty of HR13 (E_HR13_ERR)stat.error;stat.maxdoublenullablePWL15Fluxunabs0? Fitted unabsorbed flux using a fixed N_H and fixed power law index 1.5 (PWL15_FLUX_UNABS_0)mW.m**-2stat.fit.paramdoublenullablee_PWL15Fluxunabs0? Lower uncertainty of PWL15Fluxunabs0 (e_PWL15_FLUX_UNABS_0_ERR)mW.m**-2stat.errordoublenullableE_PWL15Fluxunabs0? Upper uncertainty of PWL15Fluxunabs0 (E_PWL15_FLUX_UNABS_0_ERR)mW.m**-2stat.error;stat.maxdoublenullablePWL15Fluxabs0? Fitted observed flux using a fixed N_H and fixed power law index 1.5 (PWL15_FLUX_ABS_0)mW.m**-2stat.fit.paramdoublenullablee_PWL15Fluxabs0? Lower uncertainty of PWL15Fluxabs0 (e_PWL15_FLUX_ABS_0_ERR)mW.m**-2stat.errordoublenullableE_PWL15Fluxabs0? Upper uncertainty of PWL15Fluxabs0 (E_PWL15_FLUX_ABS_0_ERR)mW.m**-2stat.error;stat.maxdoublenullablePWL15Cvar? Variance of Cash statistics of fixed N_H and fixed power law index 1.5 fit according to Kaastra et ai., 2017A&A...605A..51K (PWL15_C_VARIANCE)stat.fit.paramdoublenullablePWL15Cash? Cash statistics of fixed N_H and fixed power law index 1.5 fit (PWL15_CASH)stat.fit.paramdoublenullablePWL15CStatTh? Theoretical Cash statistics while using a fixed N_H and fixed power law index 1.5 fit according to Kaastra et ai., 2017A&A...605A..51K (PWL15_CSTAT_THEORY)stat.fit.paramdoublenullablePWL15redCash? Reduced Cash statistics from fit with fixed N_H and fixed power law index 1.5 (PWL15_REDCASH)stat.fit.paramdoublenullablePWL15CashBinsNumber of bins used during the fixed N_H and fixed power law index 1.5 fit (PWL15_CASHBINS)stat.fit.paramPWL15CashParNumber of parameters used during the fixed N_H and fixed power law index 1.5 fit (PWL15_CASHPAR)stat.fit.paramPWL15NumBinsNumber of bins used to calculate Kaastra et ai., 2017A&A...605A..51K values of fixed N_H and fixed power law index 1.5 (PWL15_NUM_BINS)stat.fit.paramPWL17Norm? Power law norm using a fixed N_H and an index of 1.7 at 1 keV (PWL17_NORM)ph.keV**-1.s**-1.cm**-2stat.fit.paramdoublenullablee_PWL17Norm? Lower uncertainty of PWL17Norm (e_PWL17_NORM_ERR)ph.keV**-1.s**-1.cm**-2stat.errordoublenullableE_PWL17Norm? Upper uncertainty of PWL17Norm (E_PWL17_NORM_ERR)ph.keV**-1.s**-1.cm**-2stat.error;stat.maxdoublenullablePWL17Fluxunabs0? Fitted unabsorbed flux using a fixed N_H and fixed power law index 1.7 (PWL17_FLUX_UNABS_0)mW.m**-2stat.fit.paramdoublenullablee_PWL17Fluxunabs0? Lower uncertainty of PWL17Fluxunabs0 (e_PWL17_FLUX_UNABS_0_ERR)mW.m**-2stat.errordoublenullableE_PWL17Fluxunabs0? Upper uncertainty of PWL17Fluxunabs0 (E_PWL17_FLUX_UNABS_0_ERR)mW.m**-2stat.error;stat.maxdoublenullablePWL17Fluxabs0? Fitted observed flux using a fixed N_H and fixed power law index 1.7 (PWL17_FLUX_ABS_0)mW.m**-2stat.fit.paramdoublenullablee_PWL17Fluxabs0? Lower uncertainty of PWL17Fluxabs0 (e_PWL17_FLUX_ABS_0_ERR)mW.m**-2stat.errordoublenullableE_PWL17Fluxabs0? Upper uncertainty of PWL17Fluxabs0 (E_PWL17_FLUX_ABS_0_ERR)mW.m**-2stat.error;stat.maxdoublenullablePWL17Cash? Cash statistics of fixed N_H and fixed power law index 1.7 fit (PWL17_CASH)stat.fit.paramdoublenullablePWL17CStatTh? Theoretical Cash statistics while using a fixed N_H and fixed power law index 1.7 fit according to Kaastra et ai., 2017A&A...605A..51K (PWL17_CSTAT_THEORY)stat.fit.paramdoublenullablePWL17redCash? Reduced Cash statistics from fit with fixed N_H and fixed power law index 1.7 (PWL17_REDCASH)stat.fit.paramdoublenullablePWL17CashBinsNumber of bins used during the fixed N_H and fixed power law index 1.7 fit (PWL17_CASHBINS)stat.fit.paramPWL17CashParNumber of parameters used during the fixed N_H and fixed power law index 1.7 fit (PWL17_CASHPAR)stat.fit.paramPWL17NumBinsNumber of bins used to calculate Kaastra et ai., 2017A&A...605A..51K values of fixed N_H and fixed power law index 1.7 (PWL17_NUM_BINS)stat.fit.paramPWL20Norm? Power law norm using a fixed N_H and an index of 2.0 at 1 keV (PWL20_NORM)ph.keV**-1.s**-1.cm**-2stat.fit.paramdoublenullablee_PWL20Norm? Lower uncertainty of PWL20Norm (e_PWL20_NORM_ERR)ph.keV**-1.s**-1.cm**-2stat.errordoublenullableE_PWL20Norm? Upper uncertainty of PWL20Norm (E_PWL20_NORM_ERR)ph.keV**-1.s**-1.cm**-2stat.error;stat.maxdoublenullablePWL20Fluxunabs0? Fitted unabsorbed flux using a fixed N_H and fixed power law index 2.0 (PWL20_FLUX_UNABS_0)mW.m**-2stat.fit.paramdoublenullablee_PWL20Fluxunabs0? Lower uncertainty of PWL20Fluxunabs0 (e_PWL20_FLUX_UNABS_0_ERR)mW.m**-2stat.errordoublenullableE_PWL20Fluxunabs0? Upper uncertainty of PWL20Fluxunabs0 (E_PWL20_FLUX_UNABS_0_ERR)mW.m**-2stat.error;stat.maxdoublenullablePWL20Fluxabs0? Fitted observed flux using a fixed N_H and fixed power law index 2.0 (PWL20_FLUX_ABS_0)mW.m**-2stat.fit.paramdoublenullablee_PWL20Fluxabs0? Lower uncertainty of PWL20Fluxabs0 (e_PWL20_FLUX_ABS_0_ERR)mW.m**-2stat.errordoublenullableE_PWL20Fluxabs0? Upper uncertainty of PWL20Fluxabs0 (E_PWL20_FLUX_ABS_0_ERR)mW.m**-2stat.error;stat.maxdoublenullablePWL20Cvar? Variance of Cash statistics of fixed N_H and fixed power law index 2.0 fit according to Kaastra et ai., 2017A&A...605A..51K (PWL20_C_VARIANCE)stat.fit.paramdoublenullablePWL20Cash? Cash statistics of fixed N_H and fixed power law index 2.0 fit (PWL20_CASH)stat.fit.paramdoublenullablePWL20CashBinsNumber of bins used during the fixed N_H and fixed power law index 2.0 fit (PWL20_CASHBINS)stat.fit.paramPWL20CashParNumber of parameters used during the fixed N_H and fixed power law index 2.0 fit (PWL20_CASHPAR)stat.fit.paramPWL20NumBinsNumber of bins used to calculate Kaastra et ai., 2017A&A...605A..51K values of fixed N_H and fixed power law index 2.0 (PWL20_NUM_BINS)stat.fit.paramPWL23Norm? Power law norm using a fixed N_H and an index of 2.3 at 1 keV (PWL23_NORM)ph.keV**-1.s**-1.cm**-2stat.fit.paramdoublenullablee_PWL23Norm? Lower uncertainty of PWL23Norm (e_PWL23_NORM_ERR)ph.keV**-1.s**-1.cm**-2stat.errordoublenullableE_PWL23Norm? Upper uncertainty of PWL23Norm (E_PWL23_NORM_ERR)ph.keV**-1.s**-1.cm**-2stat.error;stat.maxdoublenullablePWL23Fluxunabs0? Fitted unabsorbed flux using a fixed N_H and fixed power law index 2.3 (PWL23_FLUX_UNABS_0)mW.m**-2stat.fit.paramdoublenullablee_PWL23Fluxunabs0? Lower uncertainty of PWL23Fluxunabs0 (e_PWL23_FLUX_UNABS_0_ERR)mW.m**-2stat.errordoublenullableE_PWL23Fluxunabs0? Upper uncertainty of PWL23Fluxunabs0 (E_PWL23_FLUX_UNABS_0_ERR)mW.m**-2stat.error;stat.maxdoublenullablePWL23Fluxabs0? Fitted observed flux using a fixed N_H and fixed power law index 2.3 (PWL23_FLUX_ABS_0)mW.m**-2stat.fit.paramdoublenullablee_PWL23Fluxabs0? Lower uncertainty of PWL23Fluxabs0 (e_PWL23_FLUX_ABS_0_ERR)mW.m**-2stat.errordoublenullableE_PWL23Fluxabs0? Upper uncertainty of PWL23Fluxabs0 (E_PWL23_FLUX_ABS_0_ERR)mW.m**-2stat.error;stat.maxdoublenullablePWL23Cvar? Variance of Cash statistics of fixed N_H and fixed power law index 2.3 fit according to Kaastra et ai., 2017A&A...605A..51K (PWL23_C_VARIANCE)stat.fit.paramdoublenullablePWL23Cash? Cash statistics of fixed N_H and fixed power law index 2.3 fit (PWL23_CASH)stat.fit.paramdoublenullablePWL23CStatTh? Theoretical Cash statistics while using a fixed N_H and fixed power law index 2.3 fit according to Kaastra et ai., 2017A&A...605A..51K (PWL23_CSTAT_THEORY)stat.fit.paramdoublenullablePWL23redCash? Reduced Cash statistics from fit with fixed N_H and fixed power law index 2.3 (PWL23_REDCASH)stat.fit.paramdoublenullablePWL23CashBinsNumber of bins used during the fixed N_H and fixed power law index 2.3 fit (PWL23_CASHBINS)stat.fit.paramPWL23CashParNumber of parameters used during the fixed N_H and fixed power law index 2.3 fit (PWL23_CASHPAR)stat.fit.paramPWL23NumBinsNumber of bins used to calculate Kaastra et ai., 2017A&A...605A..51K values of fixed N_H and fixed power law index 2.3 (PWL23_NUM_BINS)stat.fit.paramFluxJY? Flux density at 1 keV derived from the norm of the fixed Gamma_X=2.0 fit (FLUX_JY)Jyphot.flux;em.X-raydoublenullables_FluxJY? Uncertainty of FLUX_JY (FLUX_JY_ERR)Jystat.error;phot.flux.densitydoublenullableFreeNH? Freely fitted N_H (FREE_NH)cm**-2stat.fit.paramdoublenullablee_FreeNH? Lower uncertainty of FreeNH (e_FREE_NH_ERR)cm**-2stat.errordoublenullableE_FreeNH? Upper uncertainty of FreeNH (E_FREE_NH_ERR)cm**-2stat.error;stat.maxdoublenullableFixedNumBinsNumber of bins used to calculate Kaastra et ai., 2017A&A...605A..51K values of fixed N_H power law fit (FIXED_NUM_BINS)stat.fit.param
J/A+A/709/A37/blazer1uThe unverified BlazEr1 catalog (slim version)MLctsP4ML source net counts in 2.0-5.0 keV band (ML_CTS_P4)ctphot.count;em.X-raydoubles_MLctsP4Uncertainty of ML_CTS_P4 (ML_CTS_P4_ERR)ctstat.errordoublee_MLctsP4Lower uncertainty of MLctsP4 (e_ML_CTS_P4_ASYM_ERR)ctstat.errordoubleE_MLctsP4Upper uncertainty of MLctsP4 (E_ML_CTS_P4_ASYM_ERR)ctstat.error;stat.maxdoubleMLRateP4ML source count rate in 2.0-5.0 keV band (ML_RATE_P4)ct/sphot.count;em.X-raydoubles_MLRateP4Uncertainty of ML_RATE_P4 (ML_RATE_P4_ERR)ct/sstat.errordoublee_MLRateP4Lower uncertainty of MLRateP4 (e_ML_RATE_P4_ASYM_ERR)ct/sstat.errordoubleE_MLRateP4Upper uncertainty of MLRateP4 (E_ML_RATE_P4_ASYM_ERR)ct/sstat.error;stat.maxdoubleMLFluxP4ML source flux in 2.0-5.0 keV band (ML_FLUX_P4)mW.m**-2phot.flux;em.X-raydoubles_MLFluxP4Uncertainty of ML_FLUX_P4 (ML_FLUX_P4_ERR)mW.m**-2stat.errordoublee_MLFluxP4Lower uncertainty of MLFluxP4 (e_ML_FLUX_P4_ASYM_ERR)mW.m**-2stat.errordoubleAPEExpP4Exposure map value at the given position in 2.0-5.0 keV band (APE_EXP_P4)stime.expodoubleAPERadP4Extraction radius in 2.0-5.0 keV band (APE_RADIUS_P4)pixphys.angSize;em.X-ray.mediumdoubleAPEPoisP4? Poisson probability that the extracted counts (APE_CTS) are background fluctuation in 2.0-5.0 keV band (APE_POIS_P4)stat.fit.goodnessdoublenullableDetLikeP5? Detection likelihood in 5.0-8.0 keV band (DET_LIKE_P5)stat.likelihooddoublenullableMLctsP5ML source net counts in 5.0-8.0 keV keV band (ML_CTS_P5)ctphot.count;em.X-raydoubles_MLctsP5Uncertainty of ML_CTS_P5 (ML_CTS_P5_ERR)ctstat.errordoublee_MLctsP5Lower uncertainty of MLctsP5 (e_ML_CTS_P5_ASYM_ERR)ctstat.errordoubleE_MLctsP5Upper uncertainty of MLctsP5 (E_ML_CTS_P5_ASYM_ERR)ctstat.error;stat.maxdoubleMLRateP5ML source count rate in 5.0-8.0 keV band (ML_RATE_P5)ct/sphot.count;em.X-raydoubles_MLRateP5Uncertainty of ML_RATE_P5 (ML_RATE_P5_ERR)ct/sstat.errordoublee_MLRateP5Lower uncertainty of MLRateP5 (e_ML_RATE_P5_ASYM_ERR)ct/sstat.errordoubleE_MLRateP5Upper uncertainty of MLRateP5 (E_ML_RATE_P5_ASYM_ERR)ct/sstat.error;stat.maxdoubles_MLFluxP5ML source flux in 5.0-8.0 keV band (ML_FLUX_P5)mW.m**-2phot.flux;em.X-ray.mediumdoubleMLFluxP5Uncertainty of ML_FLUX_P5 (ML_FLUX_P5_ERR)mW.m**-2phot.flux;em.X-raydoublee_MLctsP6Lower uncertainty of MLctsP6 (e_ML_CTS_P6_ASYM_ERR)ctstat.errordoubleE_MLctsP6Upper uncertainty of MLctsP6 (E_ML_CTS_P6_ASYM_ERR)ctstat.error;stat.maxdoubleMLRateP6ML source count rate in 4.0-10.0 keV band (ML_RATE_P6)ct/sphot.count;em.X-raydoubles_MLRateP6Uncertainty of ML_RATE_P6 (ML_RATE_P6_ERR)ct/sstat.errordoublee_MLRateP6Lower uncertainty of MLRateP6 (e_ML_RATE_P6_ASYM_ERR)ct/sstat.errordoubleE_MLRateP6Upper uncertainty of MLRateP6 (E_ML_RATE_P6_ASYM_ERR)ct/sstat.error;stat.maxdoubleMLFluxP6ML source flux in 4.0-10.0 keV band (ML_FLUX_P6)mW.m**-2phot.flux;em.X-raydoubles_MLFluxP6Uncertainty of ML_FLUX_P6 (ML_FLUX_P6_ERR)mW.m**-2stat.errordoublee_MLFluxP6Lower uncertainty of MLFluxP6 (e_ML_FLUX_P6_ASYM_ERR)mW.m**-2stat.errordoubleE_MLFluxP6Upper uncertainty of MLFluxP6 (E_ML_FLUX_P6_ASYM_ERR)mW.m**-2stat.error;stat.maxdoubleMLBkgP6ML background counts at the source position in 4.0-10.0 keV band (ML_BKG_P6)arcmin**-2instr.backgrounddoubleMLEefP6ML enclosed energy fraction in 4.0-10.0 keV band (ML_EEF_P6)phys.energydoubleAPEctsP6Total counts extracted within the aperture in 4.0-10.0 keV band (APE_CTS_P6)ctphot.count;em.X-rayintAPEBkgP6Background counts extracted within the aperture, excluding nearby sources using the source map in 4.0-10.0 keV band (APE_BKG_P6)ctinstr.backgrounddoubleAPEExpP6Exposure map value at the given position in 4.0-10.0 keV band (APE_EXP_P6)stime.expodoubleAPERadP6Extraction radius in 4.0-10.0 keV band (APE_RADIUS_P6)pixphys.angSize;em.X-ray.mediumdoubleAPEPoisP6? Poisson probability that the extracted counts (APE_CTS) are background fluctuation in 4.0-10.0 keV band (APE_POIS_P6)stat.fit.goodnessdoublenullableDetLikeP7? Detection likelihood in 5.1-6.1 keV band (DET_LIKE_P7)stat.likelihooddoublenullableMLctsP7ML source net counts in 5.1-6.1 keV band (ML_CTS_P7)ctphot.count;em.X-raydoubles_MLctsP7Uncertainty of ML_CTS_P7 (ML_CTS_P7_ERR)ctstat.errordoublee_MLctsP7Lower uncertainty of MLctsP7 (e_ML_CTS_P7_ASYM_ERR)ctstat.errordoubleE_MLctsP7Upper uncertainty of MLctsP7 (E_ML_CTS_P7_ASYM_ERR)ctstat.error;stat.maxdoubleMLRateP7ML source count rate in 5.1-6.1 keV band (ML_RATE_P7)ct/sphot.count;em.X-raydoubles_MLRateP7Uncertainty of ML_RATE_P7 (ML_RATE_P7_ERR)ct/sstat.errordoublee_MLRateP7Lower uncertainty of MLRateP7 (e_ML_RATE_P7_ASYM_ERR)ct/sstat.errordoubleE_MLRateP7Upper uncertainty of MLRateP7 (E_ML_RATE_P7_ASYM_ERR)ct/sstat.error;stat.maxdoubleMLFluxP7ML source flux in 5.1-6.1 keV band (ML_FLUX_P7)mW.m**-2phot.flux;em.X-raydoubles_MLFluxP7Uncertainty of ML_FLUX_P7 (ML_FLUX_P7_ERR)mW.m**-2stat.errordoublee_MLFluxP7Lower uncertainty of MLFluxP7 (e_ML_FLUX_P7_ASYM_ERR)mW.m**-2stat.errordoubleE_MLFluxP7Upper uncertainty of MLFluxP7 (E_ML_FLUX_P7_ASYM_ERR)mW.m**-2stat.error;stat.maxdoubleMLBkgP7ML background counts at the source position in 5.1-6.1 keV band (ML_BKG_P7)arcmin**-2instr.backgrounddoubleMLExpP7ML vignetted exposure time at the source position in 5.1-6.1 keV band (ML_EXP_P7)stime.duration;obs.exposuredoubleMLEefP7ML enclosed energy fraction in 5.1-6.1 keV band (ML_EEF_P7)phys.energydoubleAPEExpP9Exposure map value at the given position in 7.2-8.2 keV band (APE_EXP_P9)stime.expodoubleAPERadP9Extraction radius in 7.2-8.2 keV band (APE_RADIUS_P9)pixphys.angSize;em.X-ray.mediumdoubleAPEPoisP9? Poisson probability that the extracted counts (APE_CTS) are background fluctuation in 7.2-8.2 keV band (APE_POIS_P9)stat.fit.goodnessdoublenullableAPEctsSTotal counts extracted within the aperture in 0.5-2.0 keV band (APE_CTS_S)ctphot.count;em.X-rayintAPEBkgSBackground counts extracted within the aperture, excluding nearby sources using the source map in 0.5-2.0 keV band (APE_BKG_S)ctinstr.backgrounddoubleAPEExpSExposure map value at the given position in 0.5-2.0 keV band (APE_EXP_S)stime.expodoubleAPEPoisSPoisson probability that the extracted counts (APE_CTS) are background fluctuation in 0.5-2.0 keV band (APE_POIS_S)stat.fit.goodnessdoubleFSPSNR[0/1] If 1, source may lie within an overdense region near a supernova remnant (FLAG_SP_SNR)meta.codeintFSPBPS[0/1] If 1, source may lie within an overdense region near a bright point source (FLAG_SP_BPS)meta.codeintFSPSCL[0/1] If 1, source may lie within an overdense region near a stellar cluster (FLAG_SP_SCL)meta.codeintFSPLGA[0/1] If 1, source may lie within an overdense region near a local large galaxy (FLAG_SP_LGA)meta.codeintFSPGCCons[0/1] If 1, source may lie within an overdense region near a galaxy cluster (FLAG_SP_GC_CONS)meta.codeintFNORADEerr[0/1] If 1, source contained no RA_DEC in the preprocessed version of the catalog (FLAG_NO_RADEC_ERR)meta.codeintFNOEXTerr[0/1] If 1, source contained no EXT in the preprocessed version of the catalog (FLAG_NO_EXT_ERR)meta.codeintFNOCTSerr[0/1] If 1, source contained no MLcts0 in the preprocessed version of the catalog (FLAG_NO_CTS_ERR)meta.codeintFOPT[0] If 1, source matched with in 15arcsec with a bright optical star, likely contaminated by optical loading (FLAG_OPT)meta.codeintcts1? Counts from spectrum in 0.2-2.3 keV band (CTS_1)ctphot.count;em.X-raydoublenullablee_cts1? Lower uncertainty of cts1 (e_CTS_1_ERR)ctstat.errordoublenullablee_HR23? Lower uncertainty of HR23 (e_HR23_ERR)stat.errordoublenullableE_HR23? Upper uncertainty of HR23 (E_HR23_ERR)stat.error;stat.maxdoublenullableHR13? Hardness ratio between 0.2-0.7 keV and 1.2-2.3 keV (HR13)phot.flux;arith.ratiodoublenullablee_HR13? Lower uncertainty of HR13 (e_HR13_ERR)stat.errordoublenullableE_HR13? Upper uncertainty of HR13 (E_HR13_ERR)stat.error;stat.maxdoublenullablePWL15Norm? Power law norm using a fixed N_H and an index of 1.5 at 1 keV (PWL15_NORM)ph.keV**-1.s**-1.cm**-2stat.fit.paramdoublenullablee_PWL15Norm? Lower uncertainty of PWL15Norm (e_PWL15_NORM_ERR)ph.keV**-1.s**-1.cm**-2stat.errordoublenullableE_PWL15Norm? Upper uncertainty of PWL15Norm (E_PWL15_NORM_ERR)ph.keV**-1.s**-1.cm**-2stat.error;stat.maxdoublenullablePWL15Fluxunabs0? Fitted unabsorbed flux using a fixed N_H and fixed power law index 1.5 (PWL15_FLUX_UNABS_0)mW.m**-2stat.fit.paramdoublenullablee_PWL15Fluxunabs0? Lower uncertainty of PWL15Fluxunabs0 (e_PWL15_FLUX_UNABS_0_ERR)mW.m**-2stat.errordoublenullableE_PWL15Fluxunabs0? Upper uncertainty of PWL15Fluxunabs0 (E_PWL15_FLUX_UNABS_0_ERR)mW.m**-2stat.error;stat.maxdoublenullablePWL15Fluxabs0? Fitted observed flux using a fixed N_H and fixed power law index 1.5 (PWL15_FLUX_ABS_0)mW.m**-2stat.fit.paramdoublenullablePWL17Fluxunabs0? Fitted unabsorbed flux using a fixed N_H and fixed power law index 1.7 (PWL17_FLUX_UNABS_0)mW.m**-2stat.fit.paramdoublenullablee_PWL17Fluxunabs0? Lower uncertainty of PWL17Fluxunabs0 (e_PWL17_FLUX_UNABS_0_ERR)mW.m**-2stat.errordoublenullableE_PWL17Fluxunabs0? Upper uncertainty of PWL17Fluxunabs0 (E_PWL17_FLUX_UNABS_0_ERR)mW.m**-2stat.error;stat.maxdoublenullablePWL17Fluxabs0? Fitted observed flux using a fixed N_H and fixed power law index 1.7 (PWL17_FLUX_ABS_0)mW.m**-2stat.fit.paramdoublenullablee_PWL17Fluxabs0? Lower uncertainty of PWL17Fluxabs0 (e_PWL17_FLUX_ABS_0_ERR)mW.m**-2stat.errordoublenullableE_PWL17Fluxabs0? Upper uncertainty of PWL17Fluxabs0 (E_PWL17_FLUX_ABS_0_ERR)mW.m**-2stat.error;stat.maxdoublenullablee_PWL20Fluxunabs0? Lower uncertainty of PWL20Fluxunabs0 (e_PWL20_FLUX_UNABS_0_ERR)mW.m**-2stat.errordoublenullableE_PWL20Fluxunabs0? Upper uncertainty of PWL20Fluxunabs0 (E_PWL20_FLUX_UNABS_0_ERR)mW.m**-2stat.error;stat.maxdoublenullablePWL20Fluxabs0? Fitted observed flux using a fixed N_H and fixed power law index 2.0 (PWL20_FLUX_ABS_0)mW.m**-2stat.fit.paramdoublenullablee_PWL20Fluxabs0? Lower uncertainty of PWL20Fluxabs0 (e_PWL20_FLUX_ABS_0_ERR)mW.m**-2stat.errordoublenullableE_PWL20Fluxabs0? Upper uncertainty of PWL20Fluxabs0 (E_PWL20_FLUX_ABS_0_ERR)mW.m**-2stat.error;stat.maxdoublenullablePWL20Cvar? Variance of Cash statistics of fixed N_H and fixed power law index 2.0 fit according to Kaastra et ai., 2017A&A...605A..51K (PWL20_C_VARIANCE)stat.fit.paramdoublenullablePWL20redCash? Reduced Cash statistics from fit with fixed N_H and fixed power law index 2.0 (PWL20_REDCASH)stat.fit.paramdoublenullablePWL20CashBinsNumber of bins used during the fixed N_H and fixed power law index 2.0 fit (PWL20_CASHBINS)stat.fit.paramPWL20CashParNumber of parameters used during the fixed N_H and fixed power law index 2.0 fit (PWL20_CASHPAR)stat.fit.paramPWL20NumBinsNumber of bins used to calculate Kaastra et ai., 2017A&A...605A..51K values of fixed N_H and fixed power law index 2.0 (PWL20_NUM_BINS)stat.fit.paramPWL23Norm? Power law norm using a fixed N_H and an index of 2.3 at 1 keV (PWL23_NORM)ph.keV**-1.s**-1.cm**-2stat.fit.paramdoublenullablee_PWL23Norm? Lower uncertainty of PWL23Norm (e_PWL23_NORM_ERR)ph.keV**-1.s**-1.cm**-2stat.errordoublenullableE_PWL23Norm? Upper uncertainty of PWL23Norm (E_PWL23_NORM_ERR)ph.keV**-1.s**-1.cm**-2stat.error;stat.maxdoublenullablePWL23Fluxunabs0? Fitted unabsorbed flux using a fixed N_H and fixed power law index 2.3 (PWL23_FLUX_UNABS_0)mW.m**-2stat.fit.paramdoublenullablee_PWL23Fluxunabs0? Lower uncertainty of PWL23Fluxunabs0 (e_PWL23_FLUX_UNABS_0_ERR)mW.m**-2stat.errordoublenullableE_PWL23Fluxunabs0? Upper uncertainty of PWL23Fluxunabs0 (E_PWL23_FLUX_UNABS_0_ERR)mW.m**-2stat.error;stat.maxdoublenullablePWL23Fluxabs0? Fitted observed flux using a fixed N_H and fixed power law index 2.3 (PWL23_FLUX_ABS_0)mW.m**-2stat.fit.paramdoublenullablee_PWL23Fluxabs0? Lower uncertainty of PWL23Fluxabs0 (e_PWL23_FLUX_ABS_0_ERR)mW.m**-2stat.errordoublenullableE_PWL23Fluxabs0? Upper uncertainty of PWL23Fluxabs0 (E_PWL23_FLUX_ABS_0_ERR)mW.m**-2stat.error;stat.maxdoublenullablePWL23Cvar? Variance of Cash statistics of fixed N_H and fixed power law index 2.3 fit according to Kaastra et ai., 2017A&A...605A..51K (PWL23_C_VARIANCE)stat.fit.paramdoublenullablePWL23Cash? Cash statistics of fixed N_H and fixed power law index 2.3 fit (PWL23_CASH)stat.fit.paramdoublenullablePWL23CStatTh? Theoretical Cash statistics while using a fixed N_H and fixed power law index 2.3 fit according to Kaastra et ai., 2017A&A...605A..51K (PWL23_CSTAT_THEORY)stat.fit.paramdoublenullablePWL23redCash? Reduced Cash statistics from fit with fixed N_H and fixed power law index 2.3 (PWL23_REDCASH)stat.fit.paramdoublenullablePWL23CashBinsNumber of bins used during the fixed N_H and fixed power law index 2.3 fit (PWL23_CASHBINS)stat.fit.paramPWL23CashParNumber of parameters used during the fixed N_H and fixed power law index 2.3 fit (PWL23_CASHPAR)stat.fit.paramPWL23NumBinsNumber of bins used to calculate Kaastra et ai., 2017A&A...605A..51K values of fixed N_H and fixed power law index 2.3 (PWL23_NUM_BINS)stat.fit.paramFluxJY? Flux density at 1 keV derived from the norm of the fixed Gamma_X=2.0 fit (FLUX_JY)Jyphot.flux;em.X-raydoublenullables_FluxJY? Uncertainty of FLUX_JY (FLUX_JY_ERR)Jystat.error;phot.flux.densitydoublenullablee_FreeGAMMA? Lower uncertainty of FreeGAMMA (e_FREE_GAMMA_ERR)stat.errordoublenullableE_FreeGAMMA? Upper uncertainty of FreeGAMMA (E_FREE_GAMMA_ERR)stat.error;stat.maxdoublenullableFreeNorm? Power law norm using a free N_H at 1 keV (FREE_NORM)ph.keV**-1.s**-1.cm**-2stat.fit.paramdoublenullablee_FreeNorm? Lower uncertainty of FreeNorm (e_FREE_NORM_ERR)ph.keV**-1.s**-1.cm**-2stat.errordoublenullableE_FreeNorm? Upper uncertainty of FreeNorm (E_FREE_NORM_ERR)ph.keV**-1.s**-1.cm**-2stat.error;stat.maxdoublenullableFreeFluxunabs0? Fitted unabsorbed flux for a free N_H power law fit in 0.2-2.3 keV band (FREE_FLUX_UNABS_0)mW.m**-2stat.fit.paramdoublenullablee_FreeFluxunabs0? Lower uncertainty of FreeFluxunabs0 (e_FREE_FLUX_UNABS_0_ERR)mW.m**-2stat.errordoublenullableE_FreeFluxunabs0? Upper uncertainty of FreeFluxunabs0 (E_FREE_FLUX_UNABS_0_ERR)mW.m**-2stat.error;stat.maxdoublenullableFreeFluxabs0? Fitted observed flux for a free N_H power law fit in 0.2-2.3 keV band (FREE_FLUX_ABS_0)mW.m**-2stat.fit.paramdoublenullablee_FreeFluxabs0? Lower uncertainty of FreeFluxabs0 (e_FREE_FLUX_ABS_0_ERR)mW.m**-2stat.errordoublenullableE_FreeFluxabs0? Upper uncertainty of FreeFluxabs0 (E_FREE_FLUX_ABS_0_ERR)mW.m**-2stat.error;stat.maxdoublenullableFreeCvar? Variance of Cash statistics of free N_H power law fit according to Kaastra et ai., 2017A&A...605A..51K (FREE_C_VARIANCE)stat.fit.paramdoublenullableFreeCash? Cash statistics of free N_H power law fit (FREE_CASH)stat.fit.paramdoublenullableFreeCStatTh? Theoretical Cash statistics while using a free N_H power law fit according to Kaastra et ai., 2017A&A...605A..51K (FREE_CSTAT_THEORY)stat.fit.paramdoublenullableFreeredCash? Reduced Cash statistics from fit with free N_H (FREE_REDCASH)stat.fit.paramdoublenullableFreeCashBinsNumber of bins used during the free N_H power law fit (FREE_CASHBINS)stat.fit.paramFreeCashParNumber of parameters used during the free N_H power law fit (FREE_CASHPAR)stat.fit.paramFreeNumBinsNumber of bins used to calculate Kaastra et ai., 2017A&A...605A..51K values of free N_H power law fit (FREE_NUM_BINS)stat.fit.paramFixedNH? Fixed N_H (FIXED_NH)cm**-2stat.fit.paramdoublenullablee_FixedNorm? Lower uncertainty of FixedNorm (e_FIXED_NORM_ERR)ph.keV**-1.s**-1.cm**-2stat.errordoublenullableE_FixedNorm? Upper uncertainty of FixedNorm (E_FIXED_NORM_ERR)ph.keV**-1.s**-1.cm**-2stat.error;stat.maxdoublenullableFixedFluxunabs0? Fitted unabsorbed flux for a fixed N_H power law fit in 0.2-2.3 keV band (FIXED_FLUX_UNABS_0)mW.m**-2stat.fit.paramdoublenullablee_FixedFluxunabs0? Lower uncertainty of FixedFluxunabs0 (e_FIXED_FLUX_UNABS_0_ERR)mW.m**-2stat.errordoublenullableE_FixedFluxunabs0? Upper uncertainty of FixedFluxunabs0 (E_FIXED_FLUX_UNABS_0_ERR)mW.m**-2stat.error;stat.maxdoublenullableFixedFluxabs0? Fitted observed flux for a fixed N_H power law fit in 0.2-2.3 keV band (FIXED_FLUX_ABS_0)mW.m**-2stat.fit.paramdoublenullablee_FixedFluxabs0? Lower uncertainty of FixedFluxabs0 (e_FIXED_FLUX_ABS_0_ERR)mW.m**-2stat.errordoublenullableE_FixedFluxabs0? Upper uncertainty of FixedFluxabs0 (E_FIXED_FLUX_ABS_0_ERR)mW.m**-2stat.error;stat.maxdoublenullableFixedCvar? Variance of Cash statistics of fixed N_H power law fit according to Kaastra et ai., 2017A&A...605A..51K (FIXED_C_VARIANCE)stat.fit.paramdoublenullableFixedCash? Cash statistics of fixed N_H power law fit (FIXED_CASH)stat.fit.paramdoublenullableFixedCStatTh? Theoretical Cash statistics while using a fixed N_H power law fit according to Kaastra et ai., 2017A&A...605A..51K (FIXED_CSTAT_THEORY)stat.fit.paramdoublenullableFixedredCash? Reduced Cash statistics from fit with fixed N_H (FIXED_REDCASH)stat.fit.paramdoublenullableFixedCashBinsNumber of bins used during the fixed N_H power law fit (FIXED_CASHBINS)stat.fit.paramFixedCashParNumber of parameters used during the fixed N_H power law fit (FIXED_CASHPAR)stat.fit.paramFixedNumBinsNumber of bins used to calculate Kaastra et ai., 2017A&A...605A..51K values of fixed N_H power law fit (FIXED_NUM_BINS)stat.fit.paramNameCommon name of the source (SRC_NAME)meta.id;meta.maincharWIBRALS2srcNameName of source if listed in WIBRaLS2 (Dabrusco et al., 2019, Cat. J/ApJS/242/4) (WIBRALS2_SRC_NAME)meta.idcharIdClusterGroup ID of sources simultaneously modeled during source detection (ID_CLUSTER)meta.id.parentintABCsrcNameName of source if listed in ABC (Paggi et al., 2020, Cat. J/A+A/641/A62) (ABC_SRC_NAME)meta.idcharBROSsrcNameName of source if listed in BROS (Itoh et al., 2020, Cat. J/ApJ/901/3) (BROS_SRC_NAME)meta.idcharSepAngular separation between catalog and eROSITA position (ANGSEP)degpos.angDistancedoubleDetUIdeROSITA unique detection ID (DETUID)meta.idcharIAUNameOfficial IAU name of the eROSITA source, 1eRASS JHHMMSS.s+DDMMSS (IAUNAME)meta.idcharSkyTileeROSITA sky tile ID (SKYTILE)obs.fieldintIdSrceROSITA source ID in each sky tile (ID_SRC)meta.idintUIdInteger unique detection ID. See Merloni et al., 2024, Cat. J/A+A/682/A34 for details (UID)meta.idRADEErrCombined positional error, raw output from PSF fitting (RADEC_ERR)arcsecstat.error;posGLONGalactic longitude of eROSITA source with applied position correction (not identical to the coordinates listed by Merloni+2024) (LII)degpos.galactic.lonGLATGalactic latitude of eROSITA source with applied position correction (not identical to the coordinates listed by Merloni+2024) (BII)degpos.galactic.latdoubleELONEquatorial longitude of eROSITA source (ELON)degpos.ecliptic.lonELATEquatorial latitude of eROSITA source (ELAT)degpos.ecliptic.latdoubleMJDModified Julian Date of the observation of the source nearest to the optical axis of eROSITA (MJD)dtime.epochdoubleb_MJDModified Julian Date of the sources' first eROSITA observation (MJD_MIN)dtime.epochdoubleB_MJDModified Julian Date of the sources' last eROSITA observation (MJD_MAX)dtime.epochdoubleDetLike0Detection likelihood in 0.2-2.3 keV band (DET_LIKE_0)stat.likelihooddoubleMLcts1? ML source net counts in 0.2-2.3 keV band (ML_CTS_1)ctphot.count;em.X-raydoublenullables_MLcts1? Uncertainty of MLcts1 (ML_CTS_1_ERR)ctstat.errordoublenullablee_MLcts1? Lower uncertainty of MLcts1 (e_ML_CTS_1_ASYM_ERR)ctstat.errordoublenullableE_MLcts1? Upper uncertainty of MLcts1 (E_ML_CTS_1_ASYM_ERR)ctstat.error;stat.maxdoublenullableMLRate1? ML source count rate in 0.2-2.3 keV band (ML_RATE_1)ct/sphot.count;em.X-raydoublenullables_MLRate1? Uncertainty of MLRate1 (ML_RATE_1_ERR)ct/sstat.errordoublenullablee_s_MLRate1? Lower uncertainty of MLRate1 (e_MLRate1_ASYM_ERR)ct/sstat.errordoublenullableE_s_MLRate1? Upper uncertainty of MLRate1 (E_ML_RATE_1_ASYM_ERR)ct/sstat.error;stat.maxdoublenullableMLFlux1ML source flux in 0.2-2.3 keV band (ML_FLUX_1)mW.m**-2phot.flux;em.X-raydoubles_MLFlux1? Uncertainty of MLFlux1 (ML_FLUX_1_ERR)mW.m**-2stat.errordoublenullableMLBkgP1ML background counts at the source position in 0.2-0.5 keV band (ML_BKG_P1)arcmin**-2instr.backgrounddoubleMLExpP1ML vignetted exposure time at the source position in 0.2-0.5 keV band (ML_EXP_P1)stime.duration;obs.exposuredoubleMLEefP1ML enclosed energy fraction in 0.2-0.5 keV band (ML_EEF_P1)phys.energydoubleAPEctsP1Total counts extracted within the aperture in 0.2-0.5 keV band (APE_CTS_P1)ctphot.count;em.X-rayintAPEBkgP1Background counts extracted within the aperture, excluding nearby sources using the source map in 0.2-0.5 keV band (APE_BKG_P1)ctinstr.backgrounddoubleAPEExpP1Exposure map value at the given position in 0.2-0.5 keV band (APE_EXP_P1)stime.expodoubleAPERadP1Extraction radius in 0.2-0.5 keV band (APE_RADIUS_P1)pixphys.angSize;em.X-ray.softdoubleAPEPoisP1? Poisson probability that the extracted counts (APE_CTS) are background fluctuation in 0.2-0.5 keV band (APE_POIS_P1)stat.fit.goodnessdoublenullableDetLikeP2Detection likelihood in 0.5-1.0 keV band (DET_LIKE_P2)stat.likelihooddoubleMLctsP2ML source net counts in 0.5-1.0 keV keV band (ML_CTS_P2)ctphot.count;em.X-raydoubles_MLctsP2Uncertainty of MLctsP2 (ML_CTS_P2_ERR)ctstat.errordoublee_MLctsP2Lower uncertainty of MLctsP2 (e_ML_CTS_P2_ASYM_ERR)ctstat.errordoubleE_MLctsP2Upper uncertainty of MLctsP2 (E_ML_CTS_P2_ASYM_ERR)ctstat.error;stat.maxdoubleMLRateP2ML source count rate in 0.5-1.0 keV band (ML_RATE_P2)ct/sphot.count;em.X-raydoubles_MLRateP2Uncertainty of MLRateP2 (ML_RATE_P2_ERR)ct/sstat.errordoublee_MLRateP2Lower uncertainty of MLRateP2 (e_MLRateP2_ASYM_ERR)ct/sstat.errordoubleE_MLRateP2Upper uncertainty of MLRateP2 (E_ML_RATE_P2_ASYM_ERR)ct/sstat.error;stat.maxdoubleMLFluxP2ML source flux in 0.5-1.0 keV keV band (ML_FLUX_P2)mW.m**-2phot.flux;em.X-raydoubles_MLFluxP2Uncertainty of MLFluxP2 (ML_FLUX_P2_ERR)mW.m**-2stat.errordoublee_MLFluxP2Lower uncertainty of MLFluxP2 (e_ML_FLUX_P2_ASYM_ERR)mW.m**-2stat.errordoubleE_MLFluxP2Upper uncertainty of MLFluxP2 (E_ML_FLUX_P2_ASYM_ERR)mW.m**-2stat.error;stat.maxdoubleMLExpP2ML vignetted exposure time at the source position in 0.5-1.0 keV band (ML_EXP_P2)stime.duration;obs.exposuredoublee_MLRateP3Lower uncertainty of MLRateP3 (e_MLRateP3_ASYM_ERR)ct/sstat.errordoubleE_MLRateP3Upper uncertainty of MLRateP3 (E_ML_RATE_P3_ASYM_ERR)ct/sstat.error;stat.maxdoubleMLFluxP3ML source flux in 1.0-2.0 keV band (ML_FLUX_P3)mW.m**-2phot.flux;em.X-raydoubles_MLFluxP3Uncertainty of MLFluxP3 (ML_FLUX_P3_ERR)mW.m**-2stat.errordoublee_MLFluxP3Lower uncertainty of MLFluxP3 (e_ML_FLUX_P3_ASYM_ERR)mW.m**-2stat.errordoubleE_MLFluxP3Upper uncertainty of MLFluxP3 (E_ML_FLUX_P3_ASYM_ERR)mW.m**-2stat.error;stat.maxdoubleMLBkgP3ML background counts at the source position in 1.0-2.0 keV band (ML_BKG_P3)arcmin**-2instr.backgrounddoubleMLExpP3ML vignetted exposure time at the source position in 1.0-2.0 keV band (ML_EXP_P3)stime.duration;obs.exposuredoubleMLEefP3ML enclosed energy fraction in 1.0-2.0 keV band (ML_EEF_P3)phys.energydoubleAPEctsP3Total counts extracted within the aperture in 1.0-2.0 keV band (APE_CTS_P3)ctphot.count;em.X-rayintAPEBkgP3Background counts extracted within the aperture, excluding nearby sources using the source map in 1.0-2.0 keV band (APE_BKG_P3)ctinstr.backgrounddoubleAPEExpP3Exposure map value at the given position in 1.0-2.0 keV band (APE_EXP_P3)stime.expodoubleE_MLFluxP4Upper uncertainty of MLFluxP4 (E_ML_FLUX_P4_ASYM_ERR)mW.m**-2stat.error;stat.maxdoubleMLBkgP4ML background counts at the source position in 2.0-5.0 keV band (ML_BKG_P4)arcmin**-2instr.backgrounddoubleMLExpP4ML vignetted exposure time at the source position in 2.0-5.0 keV band (ML_EXP_P4)stime.duration;obs.exposuredoubleMLEefP4ML enclosed energy fraction in 2.0-5.0 keV band (ML_EEF_P4)phys.energydoubleAPEctsP4Total counts extracted within the aperture in 2.0-5.0 keV band (APE_CTS_P4)ctphot.count;em.X-rayintAPEBkgP4Background counts extracted within the aperture, excluding nearby sources using the source map in 2.0-5.0 keV band (APE_BKG_P4)ctinstr.backgrounddoublee_MLFluxP5Lower uncertainty of MLFluxP5 (e_ML_FLUX_P5_ASYM_ERR)mW.m**-2stat.errordoubleE_MLFluxP5Upper uncertainty of MLFluxP5 (E_ML_FLUX_P5_ASYM_ERR)mW.m**-2stat.error;stat.maxdoubleMLBkgP5ML background counts at the source position in 5.0-8.0 keV band (ML_BKG_P5)arcmin**-2instr.backgrounddoubleMLExpP5ML vignetted exposure time at the source position in 5.0-8.0 keV band (ML_EXP_P5)stime.duration;obs.exposuredoubleMLEefP5ML enclosed energy fraction in 5.0-8.0 keV band (ML_EEF_P5)phys.energydoubleAPEctsP5Total counts extracted within the aperture in 5.0-8.0 keV band (APE_CTS_P5)ctphot.count;em.X-rayintAPEBkgP5Background counts extracted within the aperture, excluding nearby sources using the source map in 5.0-8.0 keV band (APE_BKG_P5)ctinstr.backgrounddoubleAPEExpP5Exposure map value at the given position in 5.0-8.0 keV band (APE_EXP_P5)stime.expodoubleAPERadP5Extraction radius in 5.0-8.0 keV band (APE_RADIUS_P5)pixphys.angSize;em.X-ray.mediumdoubleAPEPoisP5? Poisson probability that the extracted counts (APE_CTS) are background fluctuation in 5.0-8.0 keV band (APE_POIS_P5)stat.fit.goodnessdoublenullableDetLikeP6? Detection likelihood in 4.0-10.0 keV band (DET_LIKE_P6)stat.likelihooddoublenullableMLctsP6ML source net counts in 4.0-10.0 keV keV band (ML_CTS_P6)ctphot.count;em.X-raydoubles_MLctsP6Uncertainty of ML_CTS_P6 (ML_CTS_P6_ERR)ctstat.errordoubleMLExpP6ML vignetted exposure time at the source position in 4.0-10.0 keV band (ML_EXP_P6)stime.duration;obs.exposuredoubleAPEctsP7Total counts extracted within the aperture in 5.1-6.1 keV band (APE_CTS_P7)ctphot.count;em.X-rayintAPEBkgP7Background counts extracted within the aperture, excluding nearby sources using the source map in 5.1-6.1 keV band (APE_BKG_P7)ctinstr.backgrounddoubleAPEExpP7Exposure map value at the given position in 5.1-6.1 keV band (APE_EXP_P7)stime.expodoubleAPERadP7Extraction radius in 5.1-6.1 keV band (APE_RADIUS_P7)pixphys.angSize;em.X-ray.mediumdoubleAPEPoisP7? Poisson probability that the extracted counts (APE_CTS) are background fluctuation in 5.1-6.1 keV band (APE_POIS_P7)stat.fit.goodnessdoublenullableDetLikeP8? Detection likelihood in 6.2-7.1 keV band (DET_LIKE_P8)stat.likelihooddoublenullableMLctsP8ML source net counts in 6.2-7.1 keV keV band (ML_CTS_P8)ctphot.count;em.X-raydoubles_MLctsP8Uncertainty of ML_CTS_P8 (ML_CTS_P8_ERR)ctstat.errordoublee_MLctsP8Lower uncertainty of MLctsP8 (e_ML_CTS_P8_ASYM_ERR)ctstat.errordoubleE_MLctsP8Upper uncertainty of MLctsP8 (E_ML_CTS_P8_ASYM_ERR)ctstat.error;stat.maxdoubles_MLRateP8ML source count rate in 6.2-7.1 keV band (ML_RATE_P8)ct/sarith.rate;phot.count;em.X-ray.mediumdoubleMLRateP8Uncertainty of ML_RATE_P8 (ML_RATE_P8_ERR)ct/sphot.count;em.X-raydoublee_MLRateP8Lower uncertainty of MLRateP8 (e_ML_RATE_P8_ASYM_ERR)ct/sstat.errordoubleE_MLRateP8Upper uncertainty of MLRateP8 (E_ML_RATE_P8_ASYM_ERR)ct/sstat.error;stat.maxdoubleMLFluxP8ML source flux in 6.2-7.1 keV band (ML_FLUX_P8)mW.m**-2phot.flux;em.X-raydoubles_MLFluxP8Uncertainty of ML_FLUX_P8 (ML_FLUX_P8_ERR)mW.m**-2stat.errordoublee_MLFluxP8Lower uncertainty of MLFluxP8 (e_ML_FLUX_P8_ASYM_ERR)mW.m**-2stat.errordoubleE_MLFluxP8Upper uncertainty of MLFluxP8 (E_ML_FLUX_P8_ASYM_ERR)mW.m**-2stat.error;stat.maxdoubleMLBkgP8ML background counts at the source position in 6.2-7.1 keV band (ML_BKG_P8)arcmin**-2instr.backgrounddoubleMLExpP8ML vignetted exposure time at the source position in 6.2-7.1 keV band (ML_EXP_P8)stime.duration;obs.exposuredoubleMLEefP8ML enclosed energy fraction in 6.2-7.1 keV band (ML_EEF_P8)phys.energydoubleAPEctsP8Total counts extracted within the aperture in 6.2-7.1 keV band (APE_CTS_P8)ctphot.count;em.X-rayintAPEBkgP8Background counts extracted within the aperture, excluding nearby sources using the source map in 6.2-7.1 keV band (APE_BKG_P8)ctinstr.backgrounddoubleAPEExpP8Exposure map value at the given position in 6.2-7.1 keV band (APE_EXP_P8)stime.expodoubleAPERadP8Extraction radius in 6.2-7.1 keV band (APE_RADIUS_P8)pixphys.angSize;em.X-ray.mediumdoubleAPEPoisP8? Poisson probability that the extracted counts (APE_CTS) are background fluctuation in 6.2-7.1 keV band (APE_POIS_P8)stat.fit.goodnessdoublenullableDetLikeP9? Detection likelihood in 7.2-8.2 keV band (DET_LIKE_P9)stat.likelihooddoublenullableMLctsP9ML source net counts in 7.2-8.2 keV keV band (ML_CTS_P9)ctphot.count;em.X-raydoubles_MLctsP9Uncertainty of ML_CTS_P9 (ML_CTS_P9_ERR)ctstat.errordoublee_MLctsP9Lower uncertainty of MLctsP9 (e_ML_CTS_P9_ASYM_ERR)ctstat.errordoubleE_MLctsP9Upper uncertainty of MLctsP9 (E_ML_CTS_P9_ASYM_ERR)ctstat.error;stat.maxdoubleMLRateP9ML source count rate in 7.2-8.2 keV band (ML_RATE_P9)ct/sphot.count;em.X-raydoubles_MLRateP9Uncertainty of ML_RATE_P9 (ML_RATE_P9_ERR)ct/sstat.errordoublee_MLRateP9Lower uncertainty of MLRateP9 (e_ML_RATE_P9_ASYM_ERR)ct/sstat.errordoubleE_MLRateP9Upper uncertainty of MLRateP9 (E_ML_RATE_P9_ASYM_ERR)ct/sstat.error;stat.maxdoubleMLFluxP9ML source flux in 7.2-8.2 keV band (ML_FLUX_P9)mW.m**-2phot.flux;em.X-raydoubles_MLFluxP9Uncertainty of ML_FLUX_P9 (ML_FLUX_P9_ERR)mW.m**-2stat.errordoublee_MLFluxP9Lower uncertainty of MLFluxP9 (e_ML_FLUX_P9_ASYM_ERR)mW.m**-2stat.errordoubleE_MLFluxP9Upper uncertainty of MLFluxP9 (E_ML_FLUX_P9_ASYM_ERR)mW.m**-2stat.error;stat.maxdoubleMLBkgP9ML background counts at the source position in 7.2-8.2 keV band (ML_BKG_P9)arcmin**-2instr.backgrounddoubleMLExpP9ML vignetted exposure time at the source position in 7.2-8.2 keV band (ML_EXP_P9)stime.duration;obs.exposuredoubleMLEefP9ML enclosed energy fraction in 7.2-8.2 keV band (ML_EEF_P9)phys.energydoubleAPEctsP9Total counts extracted within the aperture in 7.2-8.2 keV band (APE_CTS_P9)ctphot.count;em.X-rayintAPEBkgP9Background counts extracted within the aperture, excluding nearby sources using the source map in 7.2-8.2 keV band (APE_BKG_P9)ctinstr.backgrounddoubleE_cts1? Upper uncertainty of cts1 (E_CTS_1_ERR)ctstat.error;stat.maxdoublenullablectsT? Counts from spectrum in 0.2-10.0 keV band (CTS_T)ctphot.count;em.X-raydoublenullablee_ctsT? Lower uncertainty of ctsT (e_CTS_T_ERR)ctstat.errordoublenullableE_ctsT? Upper uncertainty of ctsT (E_CTS_T_ERR)ctstat.error;stat.maxdoublenullableSpecExpTime? Exposure time as given in the spectrum (SPEC_EXPOTIME)stime.duration;obs.exposuredoublenullableExpTimeExposure time from the eROSITA exposure map in 0.2-2.3 keV band (EXPOTIME)stime.duration;obs.exposuredoubleMinFlux95Minimum detectable flux at source position to guarantee 95% detection rate with a DetLike0 of 10 or greater in the 0.2-2.3 keV band (MIN_FLUX_95)mW.m**-2phot.flux;em.X-raydoubleAverageNH? Average N_H from the Hi4pi collaboration, 2016, Cat. J/A+A/594/A116 (AVERAGE_NH)cm**-2phys.columnDensitydoublenullableWEAverageNH? Weighted average N_H from the Hi4pi collaboration, 2016, Cat. J/A+A/594/A116 (WE_AVERAGE_NH)cm**-2phys.columnDensitydoublenullableHR12? Hardness ratio between 0.2-0.7 keV and 0.7-1.2 keV (HR12)phot.flux;arith.ratiodoublenullablee_HR12? Lower uncertainty of HR12 (e_HR12_ERR)stat.errordoublenullableE_HR12? Upper uncertainty of HR12 (E_HR12_ERR)stat.error;stat.maxdoublenullableHR23? Hardness ratio between 0.7-1.2 keV and 1.2-2.3 keV (HR23)phot.flux;arith.ratiodoublenullablee_PWL15Fluxabs0? Lower uncertainty of PWL15Fluxabs0 (e_PWL15_FLUX_ABS_0_ERR)mW.m**-2stat.errordoublenullableE_PWL15Fluxabs0? Upper uncertainty of PWL15Fluxabs0 (E_PWL15_FLUX_ABS_0_ERR)mW.m**-2stat.error;stat.maxdoublenullablePWL15Cvar? Variance of Cash statistics of fixed N_H and fixed power law index 1.5 fit according to Kaastra et ai., 2017A&A...605A..51K (PWL15_C_VARIANCE)stat.fit.paramdoublenullablePWL15Cash? Cash statistics of fixed N_H and fixed power law index 1.5 fit (PWL15_CASH)stat.fit.paramdoublenullablePWL15CStatTh? Theoretical Cash statistics while using a fixed N_H and fixed power law index 1.5 fit according to Kaastra et ai., 2017A&A...605A..51K (PWL15_CSTAT_THEORY)stat.fit.paramdoublenullablePWL15redCash? Reduced Cash statistics from fit with fixed N_H and fixed power law index 1.5 (PWL15_REDCASH)stat.fit.paramdoublenullablePWL15CashBinsNumber of bins used during the fixed N_H and fixed power law index 1.5 fit (PWL15_CASHBINS)stat.fit.paramPWL15CashParNumber of parameters used during the fixed N_H and fixed power law index 1.5 fit (PWL15_CASHPAR)stat.fit.paramPWL15NumBinsNumber of bins used to calculate Kaastra et ai., 2017A&A...605A..51K values of fixed N_H and fixed power law index 1.5 (PWL15_NUM_BINS)stat.fit.paramPWL17Norm? Power law norm using a fixed N_H and an index of 1.7 at 1 keV (PWL17_NORM)ph.keV**-1.s**-1.cm**-2stat.fit.paramdoublenullablee_PWL17Norm? Lower uncertainty of PWL17Norm (e_PWL17_NORM_ERR)ph.keV**-1.s**-1.cm**-2stat.errordoublenullableE_PWL17Norm? Upper uncertainty of PWL17Norm (E_PWL17_NORM_ERR)ph.keV**-1.s**-1.cm**-2stat.error;stat.maxdoublenullablePWL17Cvar? Variance of Cash statistics of fixed N_H and fixed power law index 1.7 fit according to Kaastra et al., 2017A&A...605A..51K (PWL17_C_VARIANCE)stat.fit.paramdoublenullablePWL17Cash? Cash statistics of fixed N_H and fixed power law index 1.7 fit (PWL17_CASH)stat.fit.paramdoublenullablePWL17CStatTh? Theoretical Cash statistics while using a fixed N_H and fixed power law index 1.7 fit according to Kaastra et ai., 2017A&A...605A..51K (PWL17_CSTAT_THEORY)stat.fit.paramdoublenullablePWL17redCash? Reduced Cash statistics from fit with fixed N_H and fixed power law index 1.7 (PWL17_REDCASH)stat.fit.paramdoublenullablePWL17CashBinsNumber of bins used during the fixed N_H and fixed power law index 1.7 fit (PWL17_CASHBINS)stat.fit.paramPWL17CashParNumber of parameters used during the fixed N_H and fixed power law index 1.7 fit (PWL17_CASHPAR)stat.fit.paramPWL17NumBinsNumber of bins used to calculate Kaastra et ai., 2017A&A...605A..51K values of fixed N_H and fixed power law index 1.7 (PWL17_NUM_BINS)stat.fit.paramPWL20Norm? Power law norm using a fixed N_H and an index of 2.0 at 1 keV (PWL20_NORM)ph.keV**-1.s**-1.cm**-2stat.fit.paramdoublenullablee_PWL20Norm? Lower uncertainty of PWL20Norm (e_PWL20_NORM_ERR)ph.keV**-1.s**-1.cm**-2stat.errordoublenullableE_PWL20Norm? Upper uncertainty of PWL20Norm (E_PWL20_NORM_ERR)ph.keV**-1.s**-1.cm**-2stat.error;stat.maxdoublenullablePWL20Fluxunabs0? Fitted unabsorbed flux using a fixed N_H and fixed power law index 2.0 (PWL20_FLUX_UNABS_0)mW.m**-2stat.fit.paramdoublenullablePWL20Cash? Cash statistics of fixed N_H and fixed power law index 2.0 fit (PWL20_CASH)stat.fit.paramdoublenullablePWL20CStatTh? Theoretical Cash statistics while using a fixed N_H and fixed power law index 2.0 fit according to Kaastra et ai., 2017A&A...605A..51K (PWL20_CSTAT_THEORY)stat.fit.paramdoublenullableFreeNH? Freely fitted N_H (FREE_NH)cm**-2stat.fit.paramdoublenullablee_FreeNH? Lower uncertainty of FreeNH (e_FREE_NH_ERR)cm**-2stat.errordoublenullableE_FreeNH? Upper uncertainty of FreeNH (E_FREE_NH_ERR)cm**-2stat.error;stat.maxdoublenullableFreeGAMMA? Power law photon index using a free N_H (FREE_GAMMA)stat.fit.paramdoublenullableFixedGAMMA? Power law photon index using a fixed N_H (FIXED_GAMMA)stat.fit.paramdoublenullablee_FixedGAMMA? Lower uncertainty of Fixed_GAMMA (e_FIXED_GAMMA_ERR)stat.errordoublenullableE_FixedGAMMA? Upper uncertainty of Fixed_GAMMA (E_FIXED_GAMMA_ERR)stat.error;stat.maxdoublenullableFixedNorm? Power law norm using a fixed N_H at 1 keV (FIXED_NORM)ph.keV**-1.s**-1.cm**-2stat.fit.paramdoublenullablerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintRAJ2000Right ascension (J2000) from input catalog (RAJ2000)degpos.eq.ra;meta.mainDEJ2000Declination (J2000) from input catalog (DECJ2000)degpos.eq.dec;meta.mainClassBlazar classification given by the input catalog (BLAZAR_CLASS)src.classcharConfBlazar[0/1] 1 for confirmed blazars and 0 for candidates (CONF_BLAZAR)meta.codeintFGLsrcNameName of source if listed in 4FGL (4FGL-DR4, Abdollahi et al., 2022, Cat. IX/67) (FGL_SRC_NAME)meta.idcharBZCATsrcNameName of source if listed in BZCAT (Massaro et al. 2015 Cat. VII/274) (BZCAT_SRC_NAME)meta.idcharHSPsrcNameName of source if listed in 3HSP (Chang et al, 2019, Cat. J/A+A/632/A77) (HSP_SRC_NAME)meta.idcharHIGHZsrcNameName of source if listed in the HighZ sample (Sbarrato et al., 2026, arXiv:2603.24659, Marcotulli et al., 2025ApJ...979L...6M) (HIGHZ_SRC_NAME)meta.idcharMILLIQUASsrcNameName of source if listed in Milliquas (Flesch et al., 2023, Cat. Cat. V/158) (MILLIQUAS_SRC_NAME)meta.idcharKDEBLLACSsrcNameName of source if listed in KDEBLLACS (Dabrusco et al., 2019, Cat. J/ApJS/242/4) (KDEBLLACS_SRC_NAME)meta.idcharUIdHardHard catalog UID of the source with a strong association, or -UID if the association is weak. 0 means no counterpart found in the Hard catalog (UID_HARD)meta.idRACdegRight ascension of eROSITA source (RA)degpos.eq.rae_RACdeg? Lower uncertainty of RA (e_RA_ERR)arcsecstat.errordoublenullableE_RACdeg? Upper uncertainty of RA (E_RA_ERR)arcsecstat.error;stat.maxdoublenullableDECdegDeclination of eROSITA source (DEC)degpos.eq.dece_DECdeg? Lower uncertainty of DEC (e_DEC_ERR)arcsecstat.errordoublenullableE_DECdeg? Upper uncertainty of DEC (E_DEC_ERR)arcsecstat.error;stat.maxdoublenullableRARdegRight ascension of eROSITA source without applying the eROSITA aspect correction (RA_RAW)degpos.eq.raDERdegDeclination of eROSITA source without applying the eROSITA aspect correction (DEC_RAW)degpos.eq.decposErr1sigma position uncertainty (POS_ERR)arcsecstat.error;posdoublee_MLFlux1? Lower uncertainty of MLFlux1 (e_ML_FLUX_1_ASYM_ERR)mW.m**-2stat.errordoublenullableE_MLFlux1? Upper uncertainty of MLFlux1 (E_ML_FLUX_1_ASYM_ERR)mW.m**-2stat.error;stat.maxdoublenullableMLBkg1ML background counts at the source position in 0.2-2.3 keV band (ML_BKG_1)arcmin**-2instr.backgrounddoubleMLExp1ML vignetted exposure time at the source position in 0.2-2.3 keV band (ML_EXP_1)stime.duration;obs.exposuredoubleMLEef1ML enclosed energy fraction in 0.2-2.3 keV band (ML_EEF_1)phys.energydoubleAPEcts1Total counts extracted within the aperture in 0.2-2.3 keV band (APE_CTS_1)ctphot.count;em.X-rayintAPEBkg1Background counts extracted within the aperture, excluding nearby sources using the source map in 0.2-2.3 keV band (APE_BKG_1)ctinstr.backgrounddoubleAPEExp1Exposure map value at the given position in 0.2-2.3 keV band (APE_EXP_1)stime.expodoubleAPERad1Extraction radius in 0.2-2.3 keV band (APE_RADIUS_1)pixphys.angSize;em.X-ray.softdoubleAPEPois1? Poisson probability that the extracted counts (APE_CTS) are background fluctuation in 0.2-2.3 keV band (APE_POIS_1)stat.fit.goodnessdoublenullableDetLikeP1? Detection likelihood in 0.2-0.5 keV band (DET_LIKE_P1)stat.likelihooddoublenullableMLctsP1ML source net counts in 0.2-0.5 keV keV band (ML_CTS_P1)ctphot.count;em.X-raydoubles_MLctsP1Uncertainty of MLctsP1 (ML_CTS_P1_ERR)ctstat.errordoublee_MLctsP1Lower uncertainty of MLctsP1 (e_ML_CTS_P1_ASYM_ERR)ctstat.errordoubleE_MLctsP1Upper uncertainty of MLctsP1 (E_ML_CTS_P1_ASYM_ERR)ctstat.error;stat.maxdoubleMLRateP1ML source count rate in 0.2-0.5 keV band (ML_RATE_P1)ct/sphot.count;em.X-raydoubles_MLRateP1Uncertainty of MLRateP1 (ML_RATE_P1_ERR)ct/sstat.errordoublee_MLRateP1Lower uncertainty of MLRateP1 (e_MLRateP1_ASYM_ERR)ct/sstat.errordoubleE_MLRateP1Upper uncertainty of MLRateP1 (E_ML_RATE_P1_ASYM_ERR)ct/sstat.error;stat.maxdoubleMLFluxP1ML source flux in 0.2-0.5 keV band (ML_FLUX_P1)mW.m**-2phot.flux;em.X-raydoubles_MLFluxP1Uncertainty of MLFluxP1 (ML_FLUX_P1_ERR)mW.m**-2stat.errordoublee_MLFluxP1Lower uncertainty of MLFluxP1 (e_ML_FLUX_P1_ASYM_ERR)mW.m**-2stat.errordoubleE_MLFluxP1Upper uncertainty of MLFluxP1 (E_ML_FLUX_P1_ASYM_ERR)mW.m**-2stat.error;stat.maxdoubleMLBkgP2ML background counts at the source position in 0.5-1.0 keV band (ML_BKG_P2)arcmin**-2instr.backgrounddoubleMLEefP2ML enclosed energy fraction in 0.5-1.0 keV band (ML_EEF_P2)phys.energydoubleAPEctsP2Total counts extracted within the aperture in 0.5-1.0 keV band (APE_CTS_P2)ctphot.count;em.X-rayintAPEBkgP2Background counts extracted within the aperture, excluding nearby sources using the source map in 0.5-1.0 keV band (APE_BKG_P2)ctinstr.backgrounddoubleAPEExpP2Exposure map value at the given position in 0.5-1.0 keV band (APE_EXP_P2)stime.expodoubleAPERadP2Extraction radius in 0.5-1.0 keV band (APE_RADIUS_P2)pixphys.angSize;em.X-ray.softdoubleAPEPoisP2? Poisson probability that the extracted counts (APE_CTS) are background fluctuation in 0.5-1.0 keV band (APE_POIS_P2)stat.fit.goodnessdoublenullableDetLikeP3Detection likelihood in 1.0-2.0 keV band (DET_LIKE_P3)stat.likelihooddoubleMLctsP3ML source net counts in 1.0-2.0 keV keV band (ML_CTS_P3)ctphot.count;em.X-raydoubles_MLctsP3Uncertainty of MLctsP3 (ML_CTS_P3_ERR)ctstat.errordoublee_MLctsP3Lower uncertainty of MLctsP3 (e_ML_CTS_P3_ASYM_ERR)ctstat.errordoubleE_MLctsP3Upper uncertainty of MLctsP3 (E_ML_CTS_P3_ASYM_ERR)ctstat.error;stat.maxdoubleMLRateP3ML source count rate in 1.0-2.0 keV band (ML_RATE_P3)ct/sphot.count;em.X-raydoubles_MLRateP3Uncertainty of MLRateP3 (ML_RATE_P3_ERR)ct/sstat.errordoubleAPERadP3Extraction radius in 1.0-2.0 keV band (APE_RADIUS_P3)pixphys.angSize;em.X-ray.softdoubleAPEPoisP3? Poisson probability that the extracted counts (APE_CTS) are background fluctuation in 1.0-2.0 keV band (APE_POIS_P3)stat.fit.goodnessdoublenullableDetLikeP4? Detection likelihood in 2.0-5.0 keV band (DET_LIKE_P4)stat.likelihooddoublenullable