J/A+A/693/A212ivo://CDS.VizieR/J/A+A/693/A212doi:10.26093/cds/vizier.36930212CDSNandra K.Waddell S.G.H.Liu T.Buchner J.Dwelly T.Salvato M.,Shen Y.Wu Q.Arcodia R.Boller T.Brunner H.Brusa M.Collmar W.,Comparat J.Georgakakis A.Grau M.Haemmerich S.Ibarra-Medel H.,Igo Z.Krumpe M.Lamer G.Merloni A.Musiimenta B.Wolf J.Assef R.J.,Bauer F.E.Brandt W.N.Rix H.-W.2025-03-03T20:01:21Z2025-01-17T08:55:21ZCDS support team

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

cds-question@unistra.frsurveysgalaxiesx-ray-sourcesDuring its calibration and performance verification phase, the eROSITA instrument aboard the Spectrum-RG satellite performed a uniform wide-area X-ray survey of approximately 140deg^2^, known as the eROSITA Final Equatorial Depth Survey (eFEDS). The primary aim of eFEDS is to demonstrate the scientific performance to be expected at the end of the eight-pass eROSITA all-sky survey. This survey will provide the first focussed image of the whole sky in the hard X-ray (>2keV) bandpass. The expected source population in this energy range is thus of great interest, particularly for AGN studies. We used a 2.3-5keV selection to construct a sample of 246 point-like hard X-ray sources for further study and characterisation. These sources are classified as either extragalactic (~90%) or Galactic (~10%), with the former consisting overwhelmingly of AGN and the latter active stars. We concentrated our further analysis on the extragalactic AGN sample, describing their X-ray and multi-wavelength properties and comparing them to the eFEDS main AGN sample selected in the softer 0.2-2.3keV band. The eROSITA hard band selects a subsample of sources that is a factor of more than ten brighter than the eFEDS main sample. The AGN within the hard population reach up to z=3.2 but on the whole, they are relatively nearby, with median z=0.34 compared to z=0.94 for the main sample. The hard survey probes typical luminosities in the range logL_X_=43-46. The X-ray spectral analysis shows significant intrinsic absorption (with logNH>21) in ~20% of the sources, with a hard X-ray power law continuum with mean <GAMMA>=1.83+/-0.04, which is typical of AGN, but slightly harder than the soft-selected eROSITA sample. Around 10% of the hard sample show a significant "soft excess" component. The sampled black hole mass distribution in the eFEDS broad-line AGN population is consistent with that of the deeper COSMOS survey that probes a higher redshift population. On the other hand, the Eddington ratios appear systematically lower, which is consistent with the idea that the decline in SMBH activity since z~1 is due to a reduction in the typical accretion rate, rather than a shift towards activity in lower-mass black holes. The eFEDS hard sample provides a preview of what can be expected from the eRASS final survey in terms of data quality. This pilot survey indicates the power of eROSITA to shed new light on the demographics and evolution of AGN, and the potential for discovery of new and rare populations.2025A&A...693A.212Nhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/693/A212CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toJ/A+A/661/A1 : The eFEDS X-ray catalogs (V7.4) (Brunner+, 2022)J/A+A/661/A3 : eFEDS counterparts to point-like sources (Salvato+, 2022)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/693/A212https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/693/A212http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/693/A212https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/693/A212https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/693/A212http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/693/A212GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/A+A/693/A212/catalog (The eFEDS hard-band selected sample)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/693/A212/catalog?https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/693/A212/catalog?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/693/A212/catalog?GETtext/xml+votable180.050000true144.2542765815891.09582488269840.0055555555555555565/1024 5459 5465 5468 6819 6822 6824-6825 6827 6830 6840 6/4100 4103-4104 4106-4109 4112-4114 4116-4118 4121-4122 4126 4128-4130 4133-4135 4137-4138 4160 4224 21830-21831 21835 21841-21845 21847 21849-21851 21853-21854 21857 21869 21876 21878-21880 21882-21885 21887 21972-21973 27269 27271 27274 27282 27292-27293 27295 27304-27306 27312-27314 27316-27317 27319 27324 27326-27327 27336 27338-27339 27364-27365 27368-27369 27371 40951 40953-40958https://cdsarc.cds.unistra.fr/viz-bin/moc/J/A+A/693/A212?format=asciiX-raydefaultJ/A+A/693/A212/catalogThe eFEDS hard-band selected samplePlatePlate (PLATE)meta.noteintzSDSSSDSS redshift (SDSS_Z)src.redshift;pos.heliocentricdoubleSNRconti? Continuum SNR (SNR_conti)stat.paramdoublenullablerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintzRedshift (Redshift)src.redshiftdoubleMLRateb10.2-0.5keV count rate (ML_RATE_b1) (1)ct/sphot.count;em.X-raydoublelogZ-m4Bayesian evidence of model 4 (logZ_m4)stat.fit.paramdoublelogLintMed-h? rest-frame 2-10keV luminosity, median, selected Model (LumiIntr_Med_h)log(1e-07W)phys.luminositydoublenullablee_Ha-br-flux? Halpha flux error (Ha_br_flux_err)mW.m**-2stat.error;phot.fluxdoublenullableIDsrc[1/28075] Source ID in this catalog (ID_SRC)meta.idintIDmain[1/26485]? The corresponding source ID in the eFEDS main catalog (ID_main)meta.idintnullableRAJ2000X-ray corrected right ascension (J2000) (RA_CORR)degpos.eq.ra;meta.mainDEJ2000X-ray corrected declination (J2000) (DEC_CORR)degpos.eq.dec;meta.mainePoaseROSITA positional uncertainty (corrected) (RADEC_ERR_CORR) (1)arcsecstat.error;posdoubleDetLike0combined three-band detection likelihood (DET_LIKE_0) (1)stat.likelihooddoubleinArea90True if in the 0.2-2.3keV exp>500s region, which comprises 90% (inArea90)meta.codedoubleDetLike10.2-0.6keV detection likelihood (DET_LIKE_1) (1)stat.likelihooddoubleDetLike20.6-2.3keV detection likelihood (DET_LIKE_2) (1)stat.likelihooddoubleDetLike32.3-5keV detection likelihood (DET_LIKE_3) (1)stat.likelihooddoubleMLRate10.2-0.6keV count rate (ML_RATE_1) (1)ct/sphot.count;em.X-raydoubleMLRate20.6-2.3keV count rate (ML_RATE_2) (1)ct/sphot.count;em.X-raydoubleMLRate32.3-5keV count rate (ML_RATE_3) (1)ct/sphot.count;em.X-raydoubleMLRateu5-8keV count rate (ML_RATE_u) (1)ct/sphot.count;em.X-raydoubleMLRateb20.5-1keV count rate (ML_RATE_b2) (1)ct/sphot.count;em.X-raydoubleMLRateb31-2keV count rate (ML_RATE_b3) (1)ct/sphot.count;em.X-raydoubleMLRateb42-4.5keV count rate (ML_RATE_b4) (1)ct/sphot.count;em.X-raydoubleMLCts10.2-0.6keV net counts (ML_CTS_1) (1)ctphot.count;em.X-raydoubleMLCts20.6-2.3keV net counts (ML_CTS_2) (1)ctphot.count;em.X-raydoubleMLCts32.3-5keV net counts (ML_CTS_3) (1)ctphot.count;em.X-raydoubleMLCtsu5-8keV net counts (ML_CTS_u) (1)ctphot.count;em.X-raydoubleMLCtsb10.2-0.5keV net counts (ML_CTS_b1) (1)ctphot.count;em.X-raydoubleMLCtsb20.5-1keV net counts (ML_CTS_b2) (1)ctphot.count;em.X-raydoubleMLCtsb31-2keV net counts (ML_CTS_b3) (1)ctphot.count;em.X-raydoubleMLCtsb42-4.5keV net counts (ML_CTS_b4) (1)ctphot.count;em.X-raydoubleMLFlux10.2-0.6keV flux (ML_FLUX_1) (1)mW.m**-2phot.flux;em.X-raydoubleMLFlux20.6-2.3keV flux (ML_FLUX_2) (1)mW.m**-2phot.flux;em.X-raydoubleMLFlux32.3-5keV flux (ML_FLUX_3) (1)mW.m**-2phot.flux;em.X-raydoubleMLFluxu5-8keV flux (ML_FLUX_u) (1)mW.m**-2phot.flux;em.X-raydoubleMLFluxb10.2-0.5keV flux (ML_FLUX_b1) (1)mW.m**-2phot.flux;em.X-raydoubleMLFluxb20.5-1keV flux (ML_FLUX_b2) (1)mW.m**-2phot.flux;em.X-raydoubleMLFluxb31-2keV flux (ML_FLUX_b3) (1)mW.m**-2phot.flux;em.X-raydoubleMLFluxb42-4.5keV flux (ML_FLUX_b4) (1)mW.m**-2phot.flux;em.X-raydoubleCTPqualCounterpart quality flag (CTP_quality) (2)meta.code.qualintCTPClass[0/3] Counterpart class, 2 for likely extraGal, 3 for secur (CTP_CLASS) (2)meta.code.classintr_zOrigin of redshift (RedshiftOrig)meta.ref;pos.framecharzGrade[2/5] Counterpart redshift grade (4 for high-quality photo-z, 5 for specz) (RedshiftGrade) (2)meta.code.qualintLS8LS8 counterpart ID (CTP_LS8_UNIQUE_OBJID)meta.idcharRALdegRight Ascension (J2000) of the LS8 counterpart (CTP_LS8_RA)degpos.eq.raDELdegDeclination (J2000) of the best LS8 counterpart (CTP_LS8_Dec)degpos.eq.decW1mag? LS8 Wise W1 magnitude (AB) (W1) (2)magphot.mag;em.IR.3-4umdoublenullablee_W1mag? LS8 Wise W1 magnitude error (W1_ERR) (2)magstat.error;phot.magdoublenullableW2mag? LS8 Wise W2 magnitude (AB) (W2) (2)magphot.mag;em.IR.4-8umdoublenullablee_W2mag? LS8 Wise W2 magnitude error (W2_ERR) (2)magstat.error;phot.magdoublenullableLS8gmag? LS8 g-band magnitude (AB) (LS8_g) (2)magphot.mag;em.opt.Bdoublenullablee_LS8gmag? LS8 g-band magnitude error (LS8_g_ERR) (2)magstat.error;phot.magdoublenullableLS8rmag? LS8 r-band magnitude (AB) (LS8_r) (2)magphot.mag;em.opt.Rdoublenullablee_LS8rmag? LS8 r-band magnitude error (LS8_r_ERR) (2)magstat.error;phot.magdoublenullableLS8zmagLS8 z-band magnitude (LS8_z) (2)magphot.mag;em.opt.Idoublee_LS8zmagLS8 z-band magnitude error (LS8_z_ERR) (2)magstat.error;phot.magdoubleinKiDS? Source is in KiDS area (in_KiDS)meta.codeintnullablegalNHTotal Galactic column density (galNH)log(cm**-2)phys.columnDensity;pos.galacticdoubleAGN[0/1] AGN subsample: CTP_CLASS>1 & inArea90 & CTP_quality>1 & RedshiftG (AGN)meta.codedoubleGammaKLm1Powerlaw slope, KL divergence (Gamma_KL_m1)stat.fit.paramdoubleb_Gammam1Powerlaw slope, 1sigma HDI lower limit (Gamma_HLo_m1)arith.grad;stat.mindoubleB_Gammam1Powerlaw slope, 1sigma HDI upper limit (Gamma_HUp_m1)arith.grad;stat.maxdoublelognHKLm1NH, KL divergence (lognH_KL_m1)log(cm**-2)phys.columnDensitydoubleb_lognHm1NH, 1sigma HDI lower limit (lognH_HLo_m1)log(cm**-2)phys.columnDensitydoubleB_lognHm1NH, 1sigma HDI upper limit (lognH_HUp_m1)log(cm**-2)phys.columnDensitydoubleFObsBF-s-m10.5-2keV observed flux, best-fit model (FluxObsv_BF_s_m1)mW.m**-2phot.flux;em.X-raydoubleFObsMed-s-m10.5-2keV observed flux, median (FluxObsv_Med_s_m1)mW.m**-2phot.flux;em.X-raydoubleb_FObs-s-m10.5-2keV observed flux, 1sigma lower limit (FluxObsv_Lo1_s_m1)mW.m**-2phot.flux;em.X-raydoubleB_FObs-s-m10.5-2keV observed flux, 1sigma upper limit (FluxObsv_Up1_s_m1)mW.m**-2phot.flux;em.X-raydoubleb2_FObs-s-m10.5-2keV observed flux, 2sigma lower limit (FluxObsv_Lo2_s_m1)mW.m**-2phot.flux;em.X-raydoubleB2_FObs-s-m10.5-2keV observed flux, 2sigma upper limit (FluxObsv_Up2_s_m1)mW.m**-2phot.flux;em.X-raydoubleFObsBF-t-m12.3-5keV observed flux, best-fit model (FluxObsv_BF_t_m1)mW.m**-2phot.flux;em.X-raydoubleFObsMed-t-m12.3-5keV observed flux, median (FluxObsv_Med_t_m1)mW.m**-2phot.flux;em.X-raydoubleb_FObs-t-m12.3-5keV observed flux, 1sigma lower limit (FluxObsv_Lo1_t_m1)mW.m**-2phot.flux;em.X-raydoubleB_FObs-t-m12.3-5keV observed flux, 1sigma upper limit (FluxObsv_Up1_t_m1)mW.m**-2phot.flux;em.X-raydoubleb2_FObs-t-m12.3-5keV observed flux, 2sigma lower limit (FluxObsv_Lo2_t_m1)mW.m**-2phot.flux;em.X-raydoubleB2_FObs-t-m12.3-5keV observed flux, 2sigma upper limit (FluxObsv_Up2_t_m1)mW.m**-2phot.flux;em.X-raydoubleFcorrBF-s-m10.5-2keV absorption corrected flux, best-fit model (FluxCorr_BF_s_m1)mW.m**-2phot.flux;em.X-raydoubleFcorrMed-s-m10.5-2keV absorption corrected flux, median (FluxCorr_Med_s_m1)mW.m**-2phot.flux;em.X-raydoubleb_Fcorr-s-m10.5-2keV absorption corrected flux, 1sigma lower limit (FluxCorr_Lo1_s_m1)mW.m**-2phot.flux;em.X-raydoubleB_Fcorr-s-m10.5-2keV absorption corrected flux, 1sigma upper limit (FluxCorr_Up1_s_m1)mW.m**-2phot.flux;em.X-raydoublelogBBNormMeanBlackbody normalization, mean (logBBNorm_Mean)stat.fit.paramdoubleb2_Fcorr-s-m10.5-2keV absorption corrected flux, 2sigma lower limit (FluxCorr_Lo2_s_m1)mW.m**-2phot.flux;em.X-raydoubleB2_Fcorr-s-m10.5-2keV absorption corrected flux, 2sigma upper limit (FluxCorr_Up2_s_m1)mW.m**-2phot.flux;em.X-raydoubleFcorrBF-t-m12.3-5keV absorption corrected flux, best-fit model (FluxCorr_BF_t_m1)mW.m**-2phot.flux;em.X-raydoubleFcorrMed-t-m12.3-5keV absorption corrected flux, median (FluxCorr_Med_t_m1)mW.m**-2phot.flux;em.X-raydoubleb_Fcorr-t-m12.3-5keV absorption corrected flux, 1sigma lower limit (FluxCorr_Lo1_t_m1)mW.m**-2phot.flux;em.X-raydoubleB_Fcorr-t-m12.3-5keV absorption corrected flux, 1sigma upper limit (FluxCorr_Up1_t_m1)mW.m**-2phot.flux;em.X-raydoubleb2_Fcorr-t-m12.3-5keV absorption corrected flux, 2sigma lower limit (FluxCorr_Lo2_t_m1)mW.m**-2phot.flux;em.X-raydoubleB2_Fcorr_t-m12.3-5keV absorption corrected flux, 2sigma upper limit (FluxCorr_Up2_t_m1)mW.m**-2phot.flux;em.X-raydoubleFintBF-s-m10.5-2keV rest-frame corrected flux, best-fit model (FluxIntr_BF_s_m1)mW.m**-2phot.flux;em.X-raydoubleFintMed-s-m10.5-2keV rest-frame corrected flux, median (FluxIntr_Med_s_m1)mW.m**-2phot.flux;em.X-raydoubleb_Fint-s-m10.5-2keV rest-frame corrected flux, 1sigma lower limit (FluxIntr_Lo1_s_m1)mW.m**-2phot.flux;em.X-raydoubleB_Fint-s-m10.5-2keV rest-frame corrected flux, 1sigma upper limit (FluxIntr_Up1_s_m1)mW.m**-2phot.flux;em.X-raydoubleb2_Fint_s-m10.5-2keV rest-frame corrected flux, 2sigma lower limit (FluxIntr_Lo2_s_m1)mW.m**-2phot.flux;em.X-raydoubleB2_Fint_s-m10.5-2keV rest-frame corrected flux, 2sigma upper limit (FluxIntr_Up2_s_m1)mW.m**-2phot.flux;em.X-raydoubleFintBF-h-m12-10keV rest-frame corrected flux, best-fit model (FluxIntr_BF_h_m1)mW.m**-2phot.flux;em.X-raydoubleFintMed-h-m12-10keV rest-frame corrected flux, median (FluxIntr_Med_h_m1)mW.m**-2phot.flux;em.X-raydoubleb_Fint-h-m12-10keV rest-frame corrected flux, 1sigma lower limit (FluxIntr_Lo1_h_m1)mW.m**-2phot.flux;em.X-raydoubleB_Fint-h-m12-10keV rest-frame corrected flux, 1sigma upper limit (FluxIntr_Up1_h_m1)mW.m**-2phot.flux;em.X-raydoubleb2_Fint-h-m12-10keV rest-frame corrected flux, 2sigma lower limit (FluxIntr_Lo2_h_m1)mW.m**-2phot.flux;em.X-raydoubleB2_Fint-h-m12-10keV rest-frame corrected flux, 2sigma upper limit (FluxIntr_Up2_h_m1)mW.m**-2phot.flux;em.X-raydoubleFintBF-2keV-m1Rest-frame 1.999-2.001keV flux, best-fit model (FluxIntr_BF_2keV_m1)mW.m**-2phot.flux;em.X-raydoubleFintMed-2keV-m1Rest-frame 1.999-2.001keV flux, median (FluxIntr_Med_2keV_m1)mW.m**-2phot.flux;em.X-raydoubleb_Fint-2keV-m1Rest-frame 1.999-2.001keV flux (FluxIntr_Lo1_2keV_m1)mW.m**-2phot.flux;em.X-raydoubleB_Fint-2keV-m1Rest-frame 1.999-2.001keV flux (FluxIntr_Up1_2keV_m1)mW.m**-2phot.flux;em.X-raydoubleb2_Fint_2keV-m1Rest-frame 1.999-2.001keV flux (FluxIntr_Lo2_2keV_m1)mW.m**-2phot.flux;em.X-raydoubleB2_Fint_2keV-m1Rest-frame 1.999-2.001keV flux (FluxIntr_Up2_2keV_m1)mW.m**-2phot.flux;em.X-raydoubleLintBF-s-m1? rest-frame 0.5-2keV luminosity, best-fit model (LumiIntr_BF_s_m1)1e-07Wphys.luminosity;em.X-raydoublenullableLintMed-s-m1? rest-frame 0.5-2keV luminosity, median (LumiIntr_Med_s_m1)1e-07Wphys.luminosity;em.X-raydoublenullableb_Lint-s-m1? rest-frame 0.5-2keV luminosity, 1sigma lower limit (LumiIntr_Lo1_s_m1)1e-07Wphys.luminosity;em.X-raydoublenullableB_Lint-s-m1? rest-frame 0.5-2keV luminosity, 1sigma upper limit (LumiIntr_Up1_s_m1)1e-07Wphys.luminosity;em.X-raydoublenullableb2_Lint-s-m1? rest-frame 0.5-2keV luminosity, 2sigma lower limit (LumiIntr_Lo2_s_m1)1e-07Wphys.luminosity;em.X-raydoublenullableB2_Lint-s-m1? rest-frame 0.5-2keV luminosity, 2sigma upper limit (LumiIntr_Up2_s_m1)1e-07Wphys.luminosity;em.X-raydoublenullableLintBF-h-m1? rest-frame 2-10keV luminosity, best-fit model (LumiIntr_BF_h_m1)1e-07Wphys.luminosity;em.X-raydoublenullableLintMed-h-m1? rest-frame 2-10keV luminosity, median (LumiIntr_Med_h_m1)1e-07Wphys.luminosity;em.X-raydoublenullableb_Lint-h-m1? rest-frame 2-10keV luminosity, 1sigma lower limit (LumiIntr_Lo1_h_m1)1e-07Wphys.luminosity;em.X-raydoublenullableB_Lint-h-m1? rest-frame 2-10keV luminosity, 1sigma upper limit (LumiIntr_Up1_h_m1)1e-07Wphys.luminosity;em.X-raydoublenullableb2_Lint-h-m1? rest-frame 2-10keV luminosity, 2sigma lower limit (LumiIntr_Lo2_h_m1)1e-07Wphys.luminosity;em.X-raydoublenullableB2_Lint-h-m1? rest-frame 2-10keV luminosity, 2sigma upper limit (LumiIntr_Up2_h_m1)1e-07Wphys.luminosity;em.X-raydoublenullableLintBF-2keV-m1? Rest-frame 1.999-2.001keV luminosity, best-fit model (LumiIntr_BF_2keV_m1)1e-07Wphys.luminosity;em.X-raydoublenullableLintMed-2keV-m1? Rest-frame 1.999-2.001keV luminosity, median (LumiIntr_Med_2keV_m1)1e-07Wphys.luminosity;em.X-raydoublenullableb_Lint-2keV-m1? Rest-frame 1.999-2.001keV luminosity, 1sigma lower limit (LumiIntr_Lo1_2keV_m1)1e-07Wphys.luminosity;em.X-raydoublenullableB_Lint-2keV-m1? Rest-frame 1.999-2.001keV luminosity, 1sigma upper limit (LumiIntr_Up1_2keV_m1)1e-07Wphys.luminosity;em.X-raydoublenullableb2_Lint2keV-m1? Rest-frame 1.999-2.001keV luminosity, 2sigma lower limit (LumiIntr_Lo2_2keV_m1)1e-07Wphys.luminosity;em.X-raydoublenullableB2_Lint2keV-m1? Rest-frame 1.999-2.001keV luminosity, 2sigma upper limit (LumiIntr_Up2_2keV_m1)1e-07Wphys.luminosity;em.X-raydoublenullableGammaMed-m1Powerlaw slope, median (Gamma_Med_m1)stat.fit.paramdoubleb_Gamma-m1Powerlaw slope, 1sigma percentile lower limit (Gamma_Lo_m1)arith.grad;stat.mindoubleB_Gamma-m1Powerlaw slope, 1sigma percentile upper limit (Gamma_Up_m1)arith.grad;stat.maxdoubleGammaMean-m1Powerlaw slope, mean (Gamma_Mean_m1)stat.fit.paramdoubleGammaStd-m1Powerlaw slope, standard deviation (Gamma_Std_m1)stat.fit.paramdoublelognHMed-m1NH, median (lognH_Med_m1)log(cm**-2)phys.columnDensitydoubleb_lognH-m1NH, 1sigma percentile lower limit (lognH_Lo_m1)log(cm**-2)phys.columnDensitydoubleB_lognH-m1NH, 1sigma percentile upper limit (lognH_Up_m1)log(cm**-2)phys.columnDensitydoublelognHMean-m1NH, mean (lognH_Mean_m1)log(cm**-2)phys.columnDensitydoublelognHStd-m1NH, standard deviation (lognH_Std_m1)log(cm**-2)phys.columnDensitydoublelogPNMed-m1Power-law normalization for AGN models, median (logPowNorm_Med_m1)stat.fit.paramdoubleb_logPN-m1Power-law normalization for AGN models, 1sigma percentile lower limit (logPowNorm_Lo_m1)stat.fit.paramdoubleB_logPN-m1Power-law normalization for AGN models, 1sigma percentile upper limit (logPowNorm_Up_m1)stat.fit.paramdoublelogPNMean-m1Power-law normalization for AGN models, mean (logPowNorm_Mean_m1)stat.fit.paramdoublelogPNStd-m1Power-law normalization for AGN models, standard deviation (logPowNorm_Std_m1)stat.fit.paramdoublelogBkgNMed-m1Background normalization, median (logBkgNorm_Med_m1)stat.fit.paramdoubleb_logBkgN-m1Background normalization, 1sigma percentile lower limit (logBkgNorm_Lo_m1)stat.fit.paramdoubleB_logBkgN-m1Background normalization, 1sigma percentile upper limit (logBkgNorm_Up_m1)stat.fit.paramdoublelogBkgNMean-m1Background normalization, mean (logBkgNorm_Mean_m1)stat.fit.paramdoublelogBkgNStd-m1Background normalization, standard deviation (logBkgNorm_Std_m1)stat.fit.paramdoublelognHKL-m0NH, KL divergence (lognH_KL_m0)log(cm**-2)phys.columnDensitydoubleNHclass[1/4] class of NH measurement, which can be 1,2,3,4 (NHclass)meta.code.classintlogZ-m1Bayesian evidence of model 1 (logZ_m1)stat.fit.paramdoubledGmKLSlope of the additional soft power law minus slope of the primary power law, KL divergence (dGm_KL)stat.fit.paramdoubleb_dGmHSlope of the additional soft power law minus slope of the primary power law, 1sigma HDI lower limit (dGm_HLo)stat.fit.paramdoubleB_dGmHSlope of the additional soft power law minus slope of the primary power law, 1sigma HDI upper limit (dGm_HUp)stat.fit.paramdoubleGammaKL-m2? Powerlaw slope, KL divergence (Gamma_KL_m2)stat.fit.paramdoublenullableb_Gamma-m2HPowerlaw slope, 1sigma HDI lower limit (Gamma_HLo_m2)arith.grad;stat.mindoubleB_Gamma-m2HPowerlaw slope, 1sigma HDI upper limit (Gamma_HUp_m2)arith.grad;stat.maxdoublelognHKL-m2NH, KL divergence (lognH_KL_m2)log(cm**-2)phys.columnDensitydoubleb_lognH-m2HNH, 1sigma HDI lower limit (lognH_HLo_m2)log(cm**-2)phys.columnDensitydoubleB_lognH-m2HNH, 1sigma HDI upper limit (lognH_HUp_m2)log(cm**-2)phys.columnDensitydoublelogFracKL? Ratio of the additional power-law to the primary power law at 1keV, KL divergence (logFrac_KL)phot.flux;arith.ratiodoublenullableb_logFracHRatio of the additional power-law to the primary power law at 1keV. 1sigma HDI lower limit (logFrac_HLo)phot.flux;arith.ratiodoubleB_logFracHRatio of the additional power-law to the primary power law at 1keV. 1sigma HDI upper limit (logFrac_HUp)phot.flux;arith.ratiodoubleFObsBF-s-m20.5-2keV observed flux, best-fit model (FluxObsv_BF_s_m2)mW.m**-2phot.flux;em.X-raydoubleFObsMed-s-m20.5-2keV observed flux, median (FluxObsv_Med_s_m2)mW.m**-2phot.flux;em.X-raydoubleb_FObs-s-m20.5-2keV observed flux, 1sigma lower limit (FluxObsv_Lo1_s_m2)mW.m**-2phot.flux;em.X-raydoubleB_FObs-s-m20.5-2keV observed flux, 1sigma upper limit (FluxObsv_Up1_s_m2)mW.m**-2phot.flux;em.X-raydoubleb2_FObs_s-m20.5-2keV observed flux, 2sigma lower limit (FluxObsv_Lo2_s_m2)mW.m**-2phot.flux;em.X-raydoubleB2_FObs_s-m20.5-2keV observed flux, 2sigma upper limit (FluxObsv_Up2_s_m2)mW.m**-2phot.flux;em.X-raydoubleFObsBF-t-m22.3-5keV observed flux, best-fit model (FluxObsv_BF_t_m2)mW.m**-2phot.flux;em.X-raydoubleFObsMed-t-m22.3-5keV observed flux, median (FluxObsv_Med_t_m2)mW.m**-2phot.flux;em.X-raydoubleb_FObs-t-m22.3-5keV observed flux, 1sigma lower limit (FluxObsv_Lo1_t_m2)mW.m**-2phot.flux;em.X-raydoubleB_FObs-t-m22.3-5keV observed flux, 1sigma upper limit (FluxObsv_Up1_t_m2)mW.m**-2phot.flux;em.X-raydoubleb2_FObs_t-m22.3-5keV observed flux, 2sigma lower limit (FluxObsv_Lo2_t_m2)mW.m**-2phot.flux;em.X-raydoubleB2_FObs_t-m22.3-5keV observed flux, 2sigma upper limit (FluxObsv_Up2_t_m2)mW.m**-2phot.flux;em.X-raydoubleFcorrBF-s-m20.5-2keV absorption corrected flux, best-fit model (FluxCorr_BF_s_m2)mW.m**-2phot.flux;em.X-raydoubleFcorrMed-s-m20.5-2keV absorption corrected flux, median (FluxCorr_Med_s_m2)mW.m**-2phot.flux;em.X-raydoubleb_Fcorr-s-m20.5-2keV absorption corrected flux, 1sigma lower limit (FluxCorr_Lo1_s_m2)mW.m**-2phot.flux;em.X-raydoubleB_Fcorr-s-m20.5-2keV absorption corrected flux, 1sigma upper limit (FluxCorr_Up1_s_m2)phot.flux;em.X-raydoubleb2_Fcorr-s-m20.5-2keV absorption corrected flux, 2sigma lower limit (FluxCorr_Lo2_s_m2)mW.m**-2phot.flux;em.X-raydoubleB2_Fcorr-s-m20.5-2keV absorption corrected flux, 2sigma upper limit (FluxCorr_Up2_s_m2)mW.m**-2phot.flux;em.X-raydoubleFcorrBF-t-m22.3-5keV absorption corrected flux, best-fit model (FluxCorr_BF_t_m2)mW.m**-2phot.flux;em.X-raydoubleFcorrMed-t-m22.3-5keV absorption corrected flux, median (FluxCorr_Med_t_m2)mW.m**-2phot.flux;em.X-raydoubleb_Fcorr-t-m22.3-5keV absorption corrected flux, 1sigma lower limit (FluxCorr_Lo1_t_m2)mW.m**-2phot.flux;em.X-raydoubleB_Fcorr-t-m22.3-5keV absorption corrected flux, 1sigma upper limit (FluxCorr_Up1_t_m2)mW.m**-2phot.flux;em.X-raydoubleb2_Fcorrt-m22.3-5keV absorption corrected flux, 2sigma lower limit (FluxCorr_Lo2_t_m2)mW.m**-2phot.flux;em.X-raydoubleB2_Fcorr_t-m22.3-5keV absorption corrected flux, 2sigma upper limit (FluxCorr_Up2_t_m2)mW.m**-2phot.flux;em.X-raydoubleFintBF-s-m20.5-2keV rest-frame corrected flux, best-fit model (FluxIntr_BF_s_m2)mW.m**-2phot.flux;em.X-raydoubleFintMed-s-m20.5-2keV rest-frame corrected flux, median (FluxIntr_Med_s_m2)mW.m**-2phot.flux;em.X-raydoubleb_Fint-s-m20.5-2keV rest-frame corrected flux, 1sigma lower limit (FluxIntr_Lo1_s_m2)mW.m**-2phot.flux;em.X-raydoubleB_Fint-s-m20.5-2keV rest-frame corrected flux, 1sigma upper limit (FluxIntr_Up1_s_m2)mW.m**-2phot.flux;em.X-raydoubleb2_Fint_s-m20.5-2keV rest-frame corrected flux, 2sigma lower limit (FluxIntr_Lo2_s_m2)mW.m**-2phot.flux;em.X-raydoubleB2_Fint_s-m20.5-2keV rest-frame corrected flux, 2sigma upper limit (FluxIntr_Up2_s_m2)mW.m**-2phot.flux;em.X-raydoubleFintBF-h-m22-10keV rest-frame corrected flux, best-fit model (FluxIntr_BF_h_m2)mW.m**-2phot.flux;em.X-raydoubleFintMed-h-m22-10keV rest-frame corrected flux, median (FluxIntr_Med_h_m2)mW.m**-2phot.flux;em.X-raydoubleb_Fint-h-m22-10keV rest-frame corrected flux, 1sigma lower limit (FluxIntr_Lo1_h_m2)mW.m**-2phot.flux;em.X-raydoubleB_Fint-h-m22-10keV rest-frame corrected flux, 1sigma upper limit (FluxIntr_Up1_h_m2)mW.m**-2phot.flux;em.X-raydoubleb2_Fint_h-m22-10keV rest-frame corrected flux, 2sigma lower limit (FluxIntr_Lo2_h_m2)mW.m**-2phot.flux;em.X-raydoubleB2_Fint_h-m22-10keV rest-frame corrected flux, 2sigma upper limit (FluxIntr_Up2_h_m2)mW.m**-2phot.flux;em.X-raydoubleFintBF-2keV-m2Rest-frame 1.999-2.001keV flux, best-fit model (FluxIntr_BF_2keV_m2)mW.m**-2phot.flux;em.X-raydoubleFintMed-2keV-m2Rest-frame 1.999-2.001keV flux, median (FluxIntr_Med_2keV_m2)mW.m**-2phot.flux;em.X-raydoubleb_Fint-2keV-m2Rest-frame 1.999-2.001keV flux (FluxIntr_Lo1_2keV_m2)mW.m**-2phot.flux;em.X-raydoubleB_Fint-2keV-m2Rest-frame 1.999-2.001keV flux (FluxIntr_Up1_2keV_m2)mW.m**-2phot.flux;em.X-raydoubleb2_Fint_2keV-m2Rest-frame 1.999-2.001keV flux (FluxIntr_Lo2_2keV_m2)mW.m**-2phot.flux;em.X-raydoubleB2_Fint_2keV-m2Rest-frame 1.999-2.001keV flux (FluxIntr_Up2_2keV_m2)mW.m**-2phot.flux;em.X-raydoublelogLintBF-s-m2? rest-frame 0.5-2keV luminosity, best-fit model (LumiIntr_BF_s_m2)log(1e-07W)phys.luminositydoublenullablelogLintMed-s-m2? rest-frame 0.5-2keV luminosity, median (LumiIntr_Med_s_m2)log(1e-07W)phys.luminositydoublenullableb_logLint-s-m2? rest-frame 0.5-2keV luminosity, 1sigma lower limit (LumiIntr_Lo1_s_m2)log(1e-07W)phys.luminosity;em.X-raydoublenullableB_logLint-s-m2? rest-frame 0.5-2keV luminosity, 1sigma upper limit (LumiIntr_Up1_s_m2)log(1e-07W)phys.luminosity;em.X-raydoublenullableb2_logLint-s-m2? rest-frame 0.5-2keV luminosity, 2sigma lower limit (LumiIntr_Lo2_s_m2)log(1e-07W)phys.luminosity;em.X-raydoublenullableB2_logLint-s-m2? rest-frame 0.5-2keV luminosity, 2sigma upper limit (LumiIntr_Up2_s_m2)log(1e-07W)phys.luminosity;em.X-raydoublenullablelogLintBF-h-m2? rest-frame 2-10keV luminosity, best-fit model (LumiIntr_BF_h_m2)log(1e-07W)phys.luminositydoublenullablelogLintMed-h-m2? rest-frame 2-10keV luminosity, median (LumiIntr_Med_h_m2)log(1e-07W)phys.luminositydoublenullableb_Lintntr-h-m2? rest-frame 2-10keV luminosity, 1sigma lower limit (LumiIntr_Lo1_h_m2)log(1e-07W)phys.luminosity;em.X-raydoublenullableB_logLint-h-m2? rest-frame 2-10keV luminosity, 1sigma upper limit (LumiIntr_Up1_h_m2)log(1e-07W)phys.luminosity;em.X-raydoublenullableb2_logLint_h-m2? rest-frame 2-10keV luminosity, 2sigma lower limit (LumiIntr_Lo2_h_m2)log(1e-07W)phys.luminosity;em.X-raydoublenullableB2_logLint_h-m2? rest-frame 2-10keV luminosity, 2sigma upper limit (LumiIntr_Up2_h_m2)log(1e-07W)phys.luminosity;em.X-raydoublenullablelogLintBF-2keV-m2? Rest-frame 1.999-2.001keV luminosity, best-fit model (LumiIntr_BF_2keV_m2)log(1e-07W)phys.luminositydoublenullablelogLintMed-2keV-m2? Rest-frame 1.999-2.001keV luminosity, median (LumiIntr_Med_2keV_m2)log(1e-07W)phys.luminositydoublenullableb_logLint-2keV-m2? Rest-frame 1.999-2.001keV luminosity, 1sigma lower limit (LumiIntr_Lo1_2keV_m2)log(1e-07W)phys.luminosity;em.X-raydoublenullableB_logLint-2keV-m2? Rest-frame 1.999-2.001keV luminosity, 1sigma upper limit (LumiIntr_Up1_2keV_m2)log(1e-07W)phys.luminosity;em.X-raydoublenullableb2_logLint-2keV-m2? Rest-frame 1.999-2.001keV luminosity, 2sigma lower limit (LumiIntr_Lo2_2keV_m2)log(1e-07W)phys.luminosity;em.X-raydoublenullableB2_logLint-2keV-m2? Rest-frame 1.999-2.001keV luminosity, 2sigma upper limit (LumiIntr_Up2_2keV_m2)log(1e-07W)phys.luminosity;em.X-raydoublenullabledGmMedSlope of the additional soft power law minus slope of the primary power law, median (dGm_Med)stat.fit.paramdoubleb_dGmSlope of the additional soft power law minus slope of the primary power law, 1sigma percentile lower limit (dGm_Lo)stat.fit.paramdoubleB_dGmSlope of the additional soft power law minus slope of the primary power law, 1sigma percentile upper limit (dGm_Up)stat.fit.paramdoubledGmMeanSlope of the additional soft power law minus slope of the primary power law, mean (dGm_Mean)stat.fit.paramdoubledGmStdSlope of the additional soft power law minus slope of the primary power law, standard deviation (dGm_Std)stat.fit.paramdoubleGammaMed-m2Powerlaw slope, median (Gamma_Med_m2)stat.fit.paramdoubleb_Gamma-m2Powerlaw slope, 1sigma percentile lower limit (Gamma_Lo_m2)arith.grad;stat.mindoubleB_Gamma-m2Powerlaw slope, 1sigma percentile upper limit (Gamma_Up_m2)arith.grad;stat.maxdoubleGammaMean-m2Powerlaw slope, mean (Gamma_Mean_m2)stat.fit.paramdoubleGammaStd-m2Powerlaw slope, standard deviation (Gamma_Std_m2)stat.fit.paramdoublelognHMed-m2NH, median (lognH_Med_m2)log(cm**-2)phys.columnDensitydoubleb_lognH-m2NH, 1sigma (lognH_Lo_m2) percentile lower limit (lognH_Lo_m2)log(cm**-2)phys.columnDensitydoubleB_lognH-m2NH, 1sigma (lognH_Up_m2) percentile upper limit (lognH_Up_m2)log(cm**-2)phys.columnDensitydoublelognH_Mean-m2NH, mean (lognH_Mean_m2)log(cm**-2)phys.columnDensitydoublelognH_Std-m2NH, standard (lognH_Std_m2) deviation (lognH_Std_m2)log(cm**-2)phys.columnDensitydoublelogPNMed-m2Power-law normalization for AGN models, median (logPowNorm_Med_m2)stat.fit.paramdoubleb_logPN-m2Power-law normalization for AGN models, 1sigma percentile lower limit (logPowNorm_Lo_m2)stat.fit.paramdoubleB_logPN-m2Power-law normalization for AGN models, 1sigma percentile upper limit (logPowNorm_Up_m2)stat.fit.paramdoublelogPNMean-m2Power-law normalization for AGN models, mean (logPowNorm_Mean_m2)stat.fit.paramdoublelogPNStd-m2Power-law normalization for AGN models, standard deviation (logPowNorm_Std_m2)stat.fit.paramdoublelogFracMedRatio of the additional power-law to the primary power law at 1keV, median (logFrac_Med)phot.flux;arith.ratiodoubleb_logFracRatio of the additional power-law to the primary power law at 1keV, 1sigma percentile lower limit (logFrac_Lo)phot.flux;arith.ratiodoubleB_logFracRatio of the additional power-law to the primary power law at 1keV, 1sigma percentile upper limit (logFrac_Up)phot.flux;arith.ratiodoublelogFracMeanRatio of the additional power-law to the primary power law at 1keV, mean (logFrac_Mean)phot.flux;arith.ratiodoublelogFracStdRatio of the additional power-law to the primary power law at 1keV, standard deviation (logFrac_Std)phot.flux;arith.ratiodoublelogBkgNMed-m2Background normalization, median (logBkgNorm_Med_m2)stat.fit.paramdoubleb_logBkgN-m2Background normalization, 1sigma percentile lower limit (logBkgNorm_Lo_m2)stat.fit.paramdoubleB_logBkgN-m2Background normalization, 1sigma percentile upper limit (logBkgNorm_Up_m2)stat.fit.paramdoublelogBkgNMean-m2Background normalization, mean (logBkgNorm_Mean_m2)stat.fit.paramdoublelogBkgNStd-m2Background normalization, standard deviation (logBkgNorm_Std_m2)stat.fit.paramdoublelogZ-m2Bayesian evidence of model 2 (logZ_m2)stat.fit.paramdoubleGammaKL-m3Powerlaw slope, KL divergence (Gamma_KL_m3)stat.fit.paramdoubleb_Gamma-m3HPowerlaw slope, 1sigma HDI lower limit (Gamma_HLo_m3)arith.grad;stat.mindoubleB_Gamma-m3HPowerlaw slope, 1sigma HDI upper limit (Gamma_HUp_m3)arith.grad;stat.maxdoublelognHKL-m3NH, KL divergence (lognH_KL_m3)log(cm**-2)phys.columnDensitydoubleb_lognH-m3HNH, 1sigma HDI lower limit (lognH_HLo_m3)log(cm**-2)phys.columnDensitydoubleB_lognH-m3HNH, 1sigma HDI upper limit (lognH_HUp_m3)log(cm**-2)phys.columnDensitydoublelogkTKL-m3Temperature of blackbody, KL divergence (logkT_KL_m3)phys.temperaturedoubleb_logkT-m3HTemperature of blackbody, 1sigma HDI lower limit (logkT_HLo_m3)phys.temperaturedoubleB_logkT-m3HTemperature of blackbody, 1sigma HDI upper limit (logkT_HUp_m3)phys.temperaturedoubleFObsBF-s-m30.5-2keV observed flux, best-fit model (FluxObsv_BF_s_m3)phot.flux;em.X-raydoubleFObsMed-s-m30.5-2keV observed flux, median (FluxObsv_Med_s_m3)phot.flux;em.X-raydoubleb_FObs-s-m30.5-2keV observed flux, 1sigma lower limit (FluxObsv_Lo1_s_m3)phot.flux;em.X-raydoubleB_FObs-s-m30.5-2keV observed flux, 1sigma upper limit (FluxObsv_Up1_s_m3)phot.flux;em.X-raydoubleb2_FObs_s-m30.5-2keV observed flux, 2sigma lower limit (FluxObsv_Lo2_s_m3)phot.flux;em.X-raydoubleB2_FObs_s-m30.5-2keV observed flux, 2sigma upper limit (FluxObsv_Up2_s_m3)phot.flux;em.X-raydoubleFObsBF-t-m32.3-5keV observed flux, best-fit model (FluxObsv_BF_t_m3)phot.flux;em.X-raydoubleFObsMed-t-m32.3-5keV observed flux, median (FluxObsv_Med_t_m3)phot.flux;em.X-raydoubleb_FObs-t-m32.3-5keV observed flux, 1sigma lower limit (FluxObsv_Lo1_t_m3)phot.flux;em.X-raydoubleB_FObs-t-m32.3-5keV observed flux, 1sigma upper limit (FluxObsv_Up1_t_m3)phot.flux;em.X-raydoubleb2_FObs_t-m32.3-5keV observed flux, 2sigma lower limit (FluxObsv_Lo2_t_m3)phot.flux;em.X-raydoubleB2_FObs_t-m32.3-5keV observed flux, 2sigma upper limit (FluxObsv_Up2_t_m3)phot.flux;em.X-raydoubleFcorrBF-s-m30.5-2keV absorption corrected flux, best-fit model (FluxCorr_BF_s_m3)phot.flux;em.X-raydoubleFcorrMed-s-m30.5-2keV absorption corrected flux, median (FluxCorr_Med_s_m3)phot.flux;em.X-raydoubleb_Fcorr-s-m30.5-2keV absorption corrected flux, 1sigma lower limit (FluxCorr_Lo1_s_m3)phot.flux;em.X-raydoubleB_Fcorr-s-m30.5-2keV absorption corrected flux, 1sigma upper limit (FluxCorr_Up1_s_m3)phot.flux;em.X-raydoubleb2_Fcorrs-m30.5-2keV absorption corrected flux, 2sigma lower limit (FluxCorr_Lo2_s_m3)phot.flux;em.X-raydoubleB2_Fcorr_s-m30.5-2keV absorption corrected flux, 2sigma upper limit (FluxCorr_Up2_s_m3)phot.flux;em.X-raydoubleFcorrBF-t-m32.3-5keV absorption corrected flux, best-fit model (FluxCorr_BF_t_m3)phot.flux;em.X-raydoubleFcorrMed-t-m32.3-5keV absorption corrected flux, median (FluxCorr_Med_t_m3)phot.flux;em.X-raydoubleb_Fcorr-t-m32.3-5keV absorption corrected flux, 1sigma lower limit (FluxCorr_Lo1_t_m3)phot.flux;em.X-raydoubleB_Fcorr-t-m32.3-5keV absorption corrected flux, 1sigma upper limit (FluxCorr_Up1_t_m3)phot.flux;em.X-raydoubleb2_Fcorr-t-m32.3-5keV absorption corrected flux, 2sigma lower limit (FluxCorr_Lo2_t_m3)phot.flux;em.X-raydoubleB2_Fcorr-t-m32.3-5keV absorption corrected flux, 2sigma upper limit (FluxCorr_Up2_t_m3)phot.flux;em.X-raydoubleFintBF-s-m30.5-2keV rest-frame corrected flux, best-fit model (FluxIntr_BF_s_m3)phot.flux;em.X-raydoubleFintMed-s-m30.5-2keV rest-frame corrected flux, median (FluxIntr_Med_s_m3)phot.flux;em.X-raydoubleb_Fint-s-m30.5-2keV rest-frame corrected flux, 1sigma lower limit (FluxIntr_Lo1_s_m3)phot.flux;em.X-raydoubleB_Fint-s-m30.5-2keV rest-frame corrected flux, 1sigma upper limit (FluxIntr_Up1_s_m3)phot.flux;em.X-raydoubleb2_Fint_s-m30.5-2keV rest-frame corrected flux, 2sigma lower limit (FluxIntr_Lo2_s_m3)phot.flux;em.X-raydoubleB2_Fint_s-m30.5-2keV rest-frame corrected flux, 2sigma upper limit (FluxIntr_Up2_s_m3)phot.flux;em.X-raydoubleFintBF-h-m32-10keV rest-frame corrected flux, best-fit model (FluxIntr_BF_h_m3)phot.flux;em.X-raydoubleFintMed-h-m32-10keV rest-frame corrected flux, median (FluxIntr_Med_h_m3)phot.flux;em.X-raydoubleb_Fint-h-m32-10keV rest-frame corrected flux, 1sigma lower limit (FluxIntr_Lo1_h_m3)phot.flux;em.X-raydoubleB_Fint-h-m32-10keV rest-frame corrected flux, 1sigma upper limit (FluxIntr_Up1_h_m3)phot.flux;em.X-raydoubleb2_Fint_h-m32-10keV rest-frame corrected flux, 2sigma lower limit (FluxIntr_Lo2_h_m3)phot.flux;em.X-raydoubleB2_Fint_h-m32-10keV rest-frame corrected flux, 2sigma upper limit (FluxIntr_Up2_h_m3)phot.flux;em.X-raydoubleFintBF-2keV-m3Rest-frame 1.999-2.001keV flux, best-fit model (FluxIntr_BF_2keV_m3)phot.flux;em.X-raydoubleFintMed-2keV-m3Rest-frame 1.999-2.001keV flux, median (FluxIntr_Med_2keV_m3)phot.flux;em.X-raydoubleb_Fint-2keV-m3Rest-frame 1.999-2.001keV flux (FluxIntr_Lo1_2keV_m3)phot.flux;em.X-raydoubleB_Fint-2keV-m3Rest-frame 1.999-2.001keV flux (FluxIntr_Up1_2keV_m3)phot.flux;em.X-raydoubleb2_Fint_2keV-m3Rest-frame 1.999-2.001keV flux (FluxIntr_Lo2_2keV_m3)phot.flux;em.X-raydoubleB2_Fint_2keV-m3Rest-frame 1.999-2.001keV flux (FluxIntr_Up2_2keV_m3)phot.flux;em.X-raydoubleLintBF-s-m3? rest-frame 0.5-2keV luminosity, best-fit model (LumiIntr_BF_s_m3)phys.luminosity;em.X-raydoublenullableLintMed-s-m3? rest-frame 0.5-2keV luminosity, median (LumiIntr_Med_s_m3)phys.luminosity;em.X-raydoublenullableb_Lint-s-m3? rest-frame 0.5-2keV luminosity, 1sigma lower limit (LumiIntr_Lo1_s_m3)phys.luminosity;em.X-raydoublenullableB_Lint-s-m3? rest-frame 0.5-2keV luminosity, 1sigma upper limit (LumiIntr_Up1_s_m3)phys.luminosity;em.X-raydoublenullableb2_Lints-m3? rest-frame 0.5-2keV luminosity, 2sigma lower limit (LumiIntr_Lo2_s_m3)phys.luminosity;em.X-raydoublenullableB2_Lints-m3? rest-frame 0.5-2keV luminosity, 2sigma upper limit (LumiIntr_Up2_s_m3)phys.luminosity;em.X-raydoublenullableLintBF-h-m3? rest-frame 2-10keV luminosity, best-fit model (LumiIntr_BF_h_m3)phys.luminosity;em.X-raydoublenullableLintMed-h-m3? rest-frame 2-10keV luminosity, median (LumiIntr_Med_h_m3)phys.luminosity;em.X-raydoublenullableb_Lint-h-m3? rest-frame 2-10keV luminosity, 1sigma lower limit (LumiIntr_Lo1_h_m3)phys.luminosity;em.X-raydoublenullableB_Lint-h-m3? rest-frame 2-10keV luminosity, 1sigma upper limit (LumiIntr_Up1_h_m3)phys.luminosity;em.X-raydoublenullableb2_Linth-m3? rest-frame 2-10keV luminosity, 2sigma lower limit (LumiIntr_Lo2_h_m3)phys.luminosity;em.X-raydoublenullableB2_Linth-m3? rest-frame 2-10keV luminosity, 2sigma upper limit (LumiIntr_Up2_h_m3)phys.luminosity;em.X-raydoublenullableLintBF-2keV-m3? Rest-frame 1.999-2.001keV luminosity, best-fit model (LumiIntr_BF_2keV_m3)phys.luminosity;em.X-raydoublenullableLintMed-2keV-m3? Rest-frame 1.999-2.001keV luminosity, median (LumiIntr_Med_2keV_m3)phys.luminosity;em.X-raydoublenullableb_Lint-2keV-m3? Rest-frame 1.999-2.001keV luminosity, 1sigma lower limit (LumiIntr_Lo1_2keV_m3)phys.luminosity;em.X-raydoublenullableB_Lint-2keV-m3? Rest-frame 1.999-2.001keV luminosity, 1sigma upper limit (LumiIntr_Up1_2keV_m3)phys.luminosity;em.X-raydoublenullableb2_Lint2keV-m3? Rest-frame 1.999-2.001keV luminosity, 2sigma lower limit (LumiIntr_Lo2_2keV_m3)phys.luminosity;em.X-raydoublenullableB2_Lint2keV-m3? Rest-frame 1.999-2.001keV luminosity, 2sigma upper limit (LumiIntr_Up2_2keV_m3)phys.luminosity;em.X-raydoublenullableGammaMed-m3Powerlaw slope, median (Gamma_Med_m3)stat.fit.paramdoubleb_Gamma-m3Powerlaw slope, 1sigma percentile lower limit (Gamma_Lo_m3)arith.grad;stat.mindoubleB_Gamma-m3Powerlaw slope, 1sigma percentile upper limit (Gamma_Up_m3)arith.grad;stat.maxdoubleGammaMean-m3Powerlaw slope, Powerlaw slope, mean (Gamma_Mean_m3)stat.fit.paramdoubleGammaStd-m3Powerlaw slope, standard deviation (Gamma_Std_m3)stat.fit.paramdoublelognHMed-m3NH, median (lognH_Med_m3)log(cm**-2)phys.columnDensitydoubleb_lognH-m3NH, 1sigma percentile lower limit (lognH_Lo_m3)log(cm**-2)phys.columnDensitydoubleB_lognH-m3NH, 1sigma percentile upper limit (lognH_Up_m3)log(cm**-2)phys.columnDensitydoublelognHMean-m3NH, mean (lognH_Mean_m3)log(cm**-2)phys.columnDensitydoublelognHStd-m3NH, standard deviation (lognH_Std_m3)log(cm**-2)phys.columnDensitydoublelogPNMed-m3Power-law normalization for AGN models, median (logPowNorm_Med_m3)stat.fit.paramdoubleb_logPN-m3Power-law normalization for AGN models, 1sigma percentile lower limit (logPowNorm_Lo_m3)stat.fit.paramdoubleB_logPN-m3Power-law normalization for AGN models, 1sigma percentile upper limit (logPowNorm_Up_m3)stat.fit.paramdoublelogPNMean-m3Power-law normalization for AGN models, mean (logPowNorm_Mean_m3)stat.fit.paramdoublelogPNStd-m3Power-law normalization for AGN models, standard deviation (logPowNorm_Std_m3)stat.fit.paramdoublelogkTMed-m3Temperature of blackbody, median (logkT_Med_m3)phys.temperaturedoubleb_logkT-m3Temperature of blackbody, 1sigma percentile lower limit (logkT_Lo_m3)phys.temperaturedoubleB_logkT-m3Temperature of blackbody, 1sigma percentile upper limit (logkT_Up_m3)phys.temperaturedoublelogkTMean-m3Temperature of blackbody, mean (logkT_Mean_m3)phys.temperaturedoublelogkTStd-m3Temperature of blackbody, standard deviation (logkT_Std_m3)phys.temperaturedoublelogBBNorm_MedBlackbody normalization, median (logBBNorm_Med)stat.fit.paramdoubleb_logBBNormBlackbody normalization, 1sigma percentile lower limit (logBBNorm_Lo)stat.fit.paramdoubleB_logBBNormBlackbody normalization, 1sigma percentile upper limit (logBBNorm_Up)stat.fit.paramdoublelogBBNormStdBlackbody normalization, standard deviation (logBBNorm_Std)stat.fit.paramdoublelogBkgNMed-m3Background normalization, median (logBkgNorm_Med_m3)stat.fit.paramdoubleb_logBkgN-m3Background normalization, 1sigma percentile lower limit (logBkgNorm_Lo_m3)stat.fit.paramdoubleB_logBkgN-m3Background normalization, 1sigma percentile upper limit (logBkgNorm_Up_m3)stat.fit.paramdoublelogBkgNMean-m3Background normalization, mean (logBkgNorm_Mean_m3)stat.fit.paramdoublelogBkgNStd-m3Background normalization, standard deviation (logBkgNorm_Std_m3)stat.fit.paramdoublelogZ-m3Bayesian evidence of model 3 (logZ_m3)stat.fit.paramdoublelognHKL-m4NH, KL divergence (lognH_KL_m4)log(cm**-2)phys.columnDensitydoubleb_logn-m4HNH, 1sigma HDI lower limit (lognH_HLo_m4)log(cm**-2)phys.columnDensitydoubleB_logn-m4HNH, 1sigma HDI upper limit (lognH_HUp_m4)log(cm**-2)phys.columnDensitydoubleFObsBF-s-m40.5-2keV observed flux, best-fit model (FluxObsv_BF_s_m4)phot.flux;em.X-raydoubleFObsMed-s-m40.5-2keV observed flux, median (FluxObsv_Med_s_m4)phot.flux;em.X-raydoubleb_FObs-s-m40.5-2keV observed flux, 1sigma lower limit (FluxObsv_Lo1_s_m4)phot.flux;em.X-raydoubleB_FObs-s-m40.5-2keV observed flux, 1sigma upper limit (FluxObsv_Up1_s_m4)phot.flux;em.X-raydoubleb2_FObs_s-m40.5-2keV observed flux, 2sigma lower limit (FluxObsv_Lo2_s_m4)phot.flux;em.X-raydoubleB2_FObs_s-m40.5-2keV observed flux, 2sigma upper limit (FluxObsv_Up2_s_m4)phot.flux;em.X-raydoubleFObsBF-t-m42.3-5keV observed flux, best-fit model (FluxObsv_BF_t_m4)phot.flux;em.X-raydoubleFObsMed-t-m42.3-5keV observed flux, median (FluxObsv_Med_t_m4)phot.flux;em.X-raydoubleb_FObs-t-m42.3-5keV observed flux, 1sigma lower limit (FluxObsv_Lo1_t_m4)phot.flux;em.X-raydoubleB_FObs-t-m42.3-5keV observed flux, 1sigma upper limit (FluxObsv_Up1_t_m4)phot.flux;em.X-raydoubleb2_FObs_t-m42.3-5keV observed flux, 2sigma lower limit (FluxObsv_Lo2_t_m4)phot.flux;em.X-raydoubleB2_FObs_t-m42.3-5keV observed flux, 2sigma upper limit (FluxObsv_Up2_t_m4)phot.flux;em.X-raydoubleFcorrBF-s-m40.5-2keV absorption corrected flux, best-fit model (FluxCorr_BF_s_m4)phot.flux;em.X-raydoubleFcorrMed-s-m40.5-2keV absorption corrected flux, median (FluxCorr_Med_s_m4)phot.flux;em.X-raydoubleb_Fcorr-s-m40.5-2keV absorption corrected flux, 1sigma lower limit (FluxCorr_Lo1_s_m4)phot.flux;em.X-raydoubleB_Fcorr-s-m40.5-2keV absorption corrected flux, 1sigma upper limit (FluxCorr_Up1_s_m4)phot.flux;em.X-raydoubleb2_Fcorr-s-m40.5-2keV absorption corrected flux, 2sigma lower limit (FluxCorr_Lo2_s_m4)phot.flux;em.X-raydoubleB2_Fcorr-s-m40.5-2keV absorption corrected flux, 2sigma upper limit (FluxCorr_Up2_s_m4)phot.flux;em.X-raydoubleFcorrBF-t-m42.3-5keV absorption corrected flux, best-fit model (FluxCorr_BF_t_m4)phot.flux;em.X-raydoubleFcorrMed-t-m42.3-5keV absorption corrected flux, median (FluxCorr_Med_t_m4)phot.flux;em.X-raydoubleb_Fcorr-t-m42.3-5keV absorption corrected flux, 1sigma lower limit (FluxCorr_Lo1_t_m4)phot.flux;em.X-raydoubleB_Fcorr-t-m42.3-5keV absorption corrected flux, 1sigma upper limit (FluxCorr_Up1_t_m4)phot.flux;em.X-raydoubleb2_Fcorrt-m42.3-5keV absorption corrected flux, 2sigma lower limit (FluxCorr_Lo2_t_m4)phot.flux;em.X-raydoubleB2_Fcorr_t-m42.3-5keV absorption corrected flux, 2sigma upper limit (FluxCorr_Up2_t_m4)phot.flux;em.X-raydoubleFintBF-s-m40.5-2keV rest-frame corrected flux, best-fit model (FluxIntr_BF_s_m4)phot.flux;em.X-raydoubleFintMed-s-m40.5-2keV rest-frame corrected flux, median (FluxIntr_Med_s_m4)phot.flux;em.X-raydoubleb_Fint-s-m40.5-2keV rest-frame corrected flux, 1sigma lower limit (FluxIntr_Lo1_s_m4)phot.flux;em.X-raydoubleB_Fint-s-m40.5-2keV rest-frame corrected flux, 1sigma upper limit (FluxIntr_Up1_s_m4)phot.flux;em.X-raydoubleb2_Fint_s-m40.5-2keV rest-frame corrected flux, 2sigma lower limit (FluxIntr_Lo2_s_m4)phot.flux;em.X-raydoubleB2_Fint_s-m40.5-2keV rest-frame corrected flux, 2sigma upper limit (FluxIntr_Up2_s_m4)phot.flux;em.X-raydoubleFintBF-h-m42-10keV rest-frame corrected flux, best-fit model (FluxIntr_BF_h_m4)phot.flux;em.X-raydoubleFintMed-h-m42-10keV rest-frame corrected flux, median (FluxIntr_Med_h_m4)phot.flux;em.X-raydoubleb_Fint-h-m42-10keV rest-frame corrected flux, 1sigma lower limit (FluxIntr_Lo1_h_m4)phot.flux;em.X-raydoubleB_Fint-h-m42-10keV rest-frame corrected flux, 1sigma upper limit (FluxIntr_Up1_h_m4)phot.flux;em.X-raydoubleb2_Fint_h-m42-10keV rest-frame corrected flux, 2sigma lower limit (FluxIntr_Lo2_h_m4)phot.flux;em.X-raydoubleB2_Fint_h-m42-10keV rest-frame corrected flux, 2sigma upper limit (FluxIntr_Up2_h_m4)phot.flux;em.X-raydoubleFintBF-2keV-m4Rest-frame 1.999-2.001keV flux, best-fit model (FluxIntr_BF_2keV_m4)phot.flux;em.X-raydoubleFintMed-2keV-m4Rest-frame 1.999-2.001keV flux, median (FluxIntr_Med_2keV_m4)phot.flux;em.X-raydoubleb_Fint-2keV-m4Rest-frame 1.999-2.001keV flux (FluxIntr_Lo1_2keV_m4)phot.flux;em.X-raydoubleB_Fint-2keV-m4Rest-frame 1.999-2.001keV flux (FluxIntr_Up1_2keV_m4)phot.flux;em.X-raydoubleb2_Fint_2keV-m4Rest-frame 1.999-2.001keV flux (FluxIntr_Lo2_2keV_m4)phot.flux;em.X-raydoubleFint_Up2_2keV-m4Rest-frame 1.999-2.001keV flux (FluxIntr_Up2_2keV_m4)phot.flux;em.X-raydoublelogLintBF-s-m4? rest-frame 0.5-2keV luminosity, best-fit model (LumiIntr_BF_s_m4)phys.luminositydoublenullablelogLintMed-s-m4? rest-frame 0.5-2keV luminosity, median (LumiIntr_Med_s_m4)phys.luminositydoublenullableb_logLint-s-m4? rest-frame 0.5-2keV luminosity, 1sigma lower limit (LumiIntr_Lo1_s_m4)phys.luminosity;em.X-raydoublenullableB_logLint-s-m4? rest-frame 0.5-2keV luminosity, 1sigma upper limit (LumiIntr_Up1_s_m4)phys.luminosity;em.X-raydoublenullableb2_logLints-m4? rest-frame 0.5-2keV luminosity, 2sigma lower limit (LumiIntr_Lo2_s_m4)phys.luminosity;em.X-raydoublenullableB2_logLints-m4? rest-frame 0.5-2keV luminosity, 2sigma upper limit (LumiIntr_Up2_s_m4)phys.luminosity;em.X-raydoublenullablelogLintBF-h-m4? rest-frame 2-10keV luminosity, best-fit model (LumiIntr_BF_h_m4)phys.luminositydoublenullablelogLintMed-h-m4? rest-frame 2-10keV luminosity, median (LumiIntr_Med_h_m4)phys.luminositydoublenullableb_logLint-h-m4? rest-frame 2-10keV luminosity, 1sigma lower limit (LumiIntr_Lo1_h_m4)phys.luminosity;em.X-raydoublenullableB_logLint-h-m4? rest-frame 2-10keV luminosity, 1sigma upper limit (LumiIntr_Up1_h_m4)phys.luminosity;em.X-raydoublenullableb2_logLinth-m4? rest-frame 2-10keV luminosity, 2sigma lower limit (LumiIntr_Lo2_h_m4)phys.luminosity;em.X-raydoublenullableB2_logLinth-m4? rest-frame 2-10keV luminosity, 2sigma upper limit (LumiIntr_Up2_h_m4)phys.luminosity;em.X-raydoublenullablelogLintBF-2keV-m4? Rest-frame 1.999-2.001keV luminosity, best-fit model (LumiIntr_BF_2keV_m4)phys.luminositydoublenullablelogLintMed-2keV-m4? Rest-frame 1.999-2.001keV luminosity, median (LumiIntr_Med_2keV_m4)phys.luminositydoublenullableb_logLint-2keV-m4? Rest-frame 1.999-2.001keV luminosity, 1sigma lower limit (LumiIntr_Lo1_2keV_m4)phys.luminosity;em.X-raydoublenullableb_lognH-m0HNH, 1sigma HDI lower limit (lognH_HLo_m0)log(cm**-2)phys.columnDensitydoubleB_logLint-2keV-m4? Rest-frame 1.999-2.001keV luminosity, 1sigma upper limit (LumiIntr_Up1_2keV_m4)phys.luminosity;em.X-raydoublenullableb2_logLint2keV-m4? Rest-frame 1.999-2.001keV luminosity, 2sigma lower limit (LumiIntr_Lo2_2keV_m4)phys.luminosity;em.X-raydoublenullableB2_logLint2keV-m4? Rest-frame 1.999-2.001keV luminosity, 2sigma upper limit (LumiIntr_Up2_2keV_m4)phys.luminosity;em.X-raydoublenullablelognHMed-m4NH, median (lognH_Med_m4)log(cm**-2)phys.columnDensitydoubleb_lognH-m4NH, 1sigma percentile lower limit (lognH_Lo_m4)log(cm**-2)phys.columnDensitydoubleB_lognH_Up-m4NH, 1sigma percentile upper limit (lognH_Up_m4)log(cm**-2)phys.columnDensitydoublelognH_Mean-m4NH, mean (lognH_Mean_m4)log(cm**-2)phys.columnDensitydoublelognH_Std-m4NH, standard deviation (lognH_Std_m4)log(cm**-2)phys.columnDensitydoublelogPNMed-m4Power-law normalization for AGN models, median (logPowNorm_Med_m4)stat.fit.paramdoubleb_logPN-m4Power-law normalization for AGN models, 1sigma percentile lower limit (logPowNorm_Lo_m4)stat.fit.paramdoubleB_logPN_Up-m4Power-law normalization for AGN models, 1sigma percentile upper limit (logPowNorm_Up_m4)stat.fit.paramdoublelogPN_Mean-m4Power-law normalization for AGN models, mean (logPowNorm_Mean_m4)stat.fit.paramdoublelogPN_Std-m4Power-law normalization for AGN models, standard deviation (logPowNorm_Std_m4)stat.fit.paramdoublelogBkgNMed-m4Background normalization, median (logBkgNorm_Med_m4)stat.fit.paramdoubleb_logBkgN-m4Background normalization, 1sigma percentile lower limit (logBkgNorm_Lo_m4)stat.fit.paramdoubleB_logBkgN_Up-m4Background normalization, 1sigma percentile upper limit (logBkgNorm_Up_m4)stat.fit.paramdoublelogBkgN_Mean-m4Background normalization, mean (logBkgNorm_Mean_m4)stat.fit.paramdoublelogBkgN_Std-m4Background normalization, standard deviation (logBkgNorm_Std_m4)stat.fit.paramdoubleGammaKL-m5Powerlaw slope, KL divergence (Gamma_KL_m5)stat.fit.paramdoubleb_Gamma-m5HPowerlaw slope, 1sigma HDI lower limit (Gamma_HLo_m5)arith.grad;stat.mindoubleB_Gamma-m5HPowerlaw slope, 1sigma HDI upper limit (Gamma_HUp_m5)arith.grad;stat.maxdoublelognHKL-m5NH, KL divergence (lognH_KL_m5)log(cm**-2)phys.columnDensitydoubleb_lognH-m5HNH, 1sigma HDI lower limit (lognH_HLo_m5)log(cm**-2)phys.columnDensitydoubleB_lognH-m5HNH, 1sigma HDI upper limit (lognH_HUp_m5)log(cm**-2)phys.columnDensitydoubleFObsBF-t-m52.3-5keV observed flux, best-fit model (FluxObsv_BF_t_m5)phot.flux;em.X-raydoubleFObsMed-t-m52.3-5keV observed flux, median (FluxObsv_Med_t_m5)phot.flux;em.X-raydoubleb_FObs-t-m52.3-5keV observed flux, 1sigma lower limit (FluxObsv_Lo1_t_m5)phot.flux;em.X-raydoubleB_FObs-t-m52.3-5keV observed flux, 1sigma upper limit (FluxObsv_Up1_t_m5)phot.flux;em.X-raydoubleb2_FObs_t-m52.3-5keV observed flux, 2sigma lower limit (FluxObsv_Lo2_t_m5)phot.flux;em.X-raydoubleB2_FObs_t-m52.3-5keV observed flux, 2sigma upper limit (FluxObsv_Up2_t_m5)phot.flux;em.X-raydoubleFcorrBF-t-m52.3-5keV absorption corrected flux, best-fit model (FluxCorr_BF_t_m5)phot.flux;em.X-raydoubleFcorrMed-t-m52.3-5keV absorption corrected flux, median (FluxCorr_Med_t_m5)phot.flux;em.X-raydoubleb_Fcorr-t-m52.3-5keV absorption corrected flux, 1sigma lower limit (FluxCorr_Lo1_t_m5)phot.flux;em.X-raydoubleB_Fcorr-t-m52.3-5keV absorption corrected flux, 1sigma upper limit (FluxCorr_Up1_t_m5)phot.flux;em.X-raydoubleb2_Fcorrt-m52.3-5keV absorption corrected flux, 2sigma lower limit (FluxCorr_Lo2_t_m5)phot.flux;em.X-raydoubleB2_Fcorrt-m52.3-5keV absorption corrected flux, 2sigma upper limit (FluxCorr_Up2_t_m5)phot.flux;em.X-raydoubleFintBF-h-m52-10keV rest-frame corrected flux, best-fit model (FluxIntr_BF_h_m5)phot.flux;em.X-raydoubleFintMed-h-m52-10keV rest-frame corrected flux, median (FluxIntr_Med_h_m5)phot.flux;em.X-raydoubleb_Fint-h-m52-10keV rest-frame corrected flux, 1sigma lower limit (FluxIntr_Lo1_h_m5)phot.flux;em.X-raydoubleB_Fint-h-m52-10keV rest-frame corrected flux, 1sigma upper limit (FluxIntr_Up1_h_m5)phot.flux;em.X-raydoubleb2_Fint_h-m52-10keV rest-frame corrected flux, 2sigma lower limit (FluxIntr_Lo2_h_m5)phot.flux;em.X-raydoubleB2_Fint_h-m52-10keV rest-frame corrected flux, 2sigma upper limit (FluxIntr_Up2_h_m5)phot.flux;em.X-raydoubleLintBF-h-m5? rest-frame 2-10keV luminosity, best-fit model (LumiIntr_BF_h_m5)phys.luminosity;em.X-raydoublenullableLintMed-h-m5? rest-frame 2-10keV luminosity, median (LumiIntr_Med_h_m5)phys.luminosity;em.X-raydoublenullableb_Lint-h-m5? rest-frame 2-10keV luminosity, 1sigma lower limit (LumiIntr_Lo1_h_m5)phys.luminosity;em.X-raydoublenullableB_Lint-h-m5? rest-frame 2-10keV luminosity, 1sigma upper limit (LumiIntr_Up1_h_m5)phys.luminosity;em.X-raydoublenullableb2_Lint-h-m5? rest-frame 2-10keV luminosity, 2sigma lower limit (LumiIntr_Lo2_h_m5)phys.luminosity;em.X-raydoublenullableB2_Lint-h-m5? rest-frame 2-10keV luminosity, 2sigma upper limit (LumiIntr_Up2_h_m5)phys.luminosity;em.X-raydoublenullableGammaMed-m5Powerlaw slope, median (Gamma_Med_m5)stat.fit.paramdoubleb_Gamma-m5Powerlaw slope, 1sigma percentile lower limit (Gamma_Lo_m5)arith.grad;stat.mindoubleB_Gamma-m5Powerlaw slope, 1sigma percentile upper limit (Gamma_Up_m5)arith.grad;stat.maxdoubleGammaMean-m5Powerlaw slope, mean (Gamma_Mean_m5)stat.fit.paramdoubleGammaStd-m5Powerlaw slope, standard deviation (Gamma_Std_m5)stat.fit.paramdoublelognHMed-m5NH, median (lognH_Med_m5)log(cm**-2)phys.columnDensitydoubleb_lognH-m5NH, 1sigma percentile lower limit (lognH_Lo_m5)log(cm**-2)phys.columnDensitydoubleB_lognH-m5NH, 1sigma percentile upper limit (lognH_Up_m5)log(cm**-2)phys.columnDensitydoublelognHMean-m5NH, mean (lognH_Mean_m5)log(cm**-2)phys.columnDensitydoublelognHStd-m5NH, standard deviation (lognH_Std_m5)log(cm**-2)phys.columnDensitydoublelogPNMed-m5Power-law normalization for AGN models, median (logPowNorm_Med_m5)stat.fit.paramdoubleb_logPN-m5Power-law normalization for AGN models, 1sigma percentile lower limit (logPowNorm_Lo_m5)stat.fit.paramdoubleB_logPN-m5Power-law normalization for AGN models, 1sigma percentile upper limit (logPowNorm_Up_m5)stat.fit.paramdoublelogPNMean-m5Power-law normalization for AGN models, mean (logPowNorm_Mean_m5)stat.fit.paramdoublelogPNStd-m5Power-law normalization for AGN models, standard deviation (logPowNorm_Std_m5)stat.fit.paramdoublelogBkgNMed-m5Background normalization, median (logBkgNorm_Med_m5)stat.fit.paramdoubleb_logBkgN-m5Background normalization, 1sigma percentile lower limit (logBkgNorm_Lo_m5)stat.fit.paramdoubleB_logBkgN-m5Background normalization, 1sigma percentile upper limit (logBkgNorm_Up_m5)stat.fit.paramdoublelogBkgNMean-m5Background normalization, mean (logBkgNorm_Mean_m5)stat.fit.paramdoublelogBkgNStd-m5Background normalization, standard deviation (logBkgNorm_Std_m5)stat.fit.paramdoublelogZ-m5Bayesian evidence of model 5 (logZ_m5)stat.fit.paramdoubleB_lognH-m0HNH, 1sigma HDI upper limit (lognH_HUp_m0)log(cm**-2)phys.columnDensitydoublelogkTKL-m0Temperature of APEC, KL divergence (logkT_KL_m0)phys.temperaturedoubleb_logkT-m0HTemperature of APEC, 1sigma HDI lower limit (logkT_HLo_m0)phys.temperaturedoubleB_logkT-m0HTemperature of APEC, 1sigma HDI upper limit (logkT_HUp_m0)phys.temperaturedoublelogAbundKLAbundance of the APEC model, KL divergence (logAbundanc_KL)phys.abunddoubleb_logAbundHAbundance of the APEC model, 1sigma HDI lower limit (logAbundanc_HLo)phys.abunddoubleB_logAbundHAbundance of the APEC model, 1sigma HDI upper limit (logAbundanc_HUp)phys.abunddoubleFObsBF-s-m00.5-2keV observed flux, best-fit model (FluxObsv_BF_s_m0)phot.flux;em.X-raydoubleFObsMed-s-m00.5-2keV observed flux, median (FluxObsv_Med_s_m0)phot.flux;em.X-raydoubleb_FObs-s-m00.5-2keV observed flux, 1sigma lower limit (FluxObsv_Lo1_s_m0)phot.flux;em.X-raydoubleB_FObs-s-m00.5-2keV observed flux, 1sigma upper limit (FluxObsv_Up1_s_m0)phot.flux;em.X-raydoubleb2_FObs_s-m00.5-2keV observed flux, 2sigma lower limit (FluxObsv_Lo2_s_m0)phot.flux;em.X-raydoubleB2_FObs_s-m00.5-2keV observed flux, 2sigma upper limit (FluxObsv_Up2_s_m0)phot.flux;em.X-raydoubleFObsBF-t-m02.3-5keV observed flux, best-fit model (FluxObsv_BF_t_m0)phot.flux;em.X-raydoubleFObsMed-t-m02.3-5keV observed flux, median (FluxObsv_Med_t_m0)phot.flux;em.X-raydoubleb_FObs-t-m02.3-5keV observed flux, 1sigma lower limit (FluxObsv_Lo1_t_m0)phot.flux;em.X-raydoubleB_FObs-t-m02.3-5keV observed flux, 1sigma upper limit (FluxObsv_Up1_t_m0)phot.flux;em.X-raydoubleb2_FObs-t-m02.3-5keV observed flux, 2sigma lower limit (FluxObsv_Lo2_t_m0)phot.flux;em.X-raydoubleB2_FObs-t-m02.3-5keV observed flux, 2sigma upper limit (FluxObsv_Up2_t_m0)phot.flux;em.X-raydoublelognHMed-m0NH, median (lognH_Med_m0)log(cm**-2)phys.columnDensitydoubleb_lognH-m0NH, 1sigma percentile lower limit (lognH_Lo_m0)log(cm**-2)phys.columnDensitydoubleB_lognH-m0NH, 1sigma percentile upper limit (lognH_Up_m0)log(cm**-2)phys.columnDensitydoublelognHMean-m0NH, mean (lognH_Mean_m0)log(cm**-2)phys.columnDensitydoublelognHStd-m0NH, standard deviation (lognH_Std_m0)log(cm**-2)phys.columnDensitydoublelogkTMed-m0Temperature of APEC, median (logkT_Med_m0)phys.temperaturedoubleb_logkT-m0Temperature of APEC, 1sigma percentile lower limit (logkT_Lo_m0)phys.temperaturedoubleB_logkT-m0Temperature of APEC, 1sigma percentile upper limit (logkT_Up_m0)phys.temperaturedoublelogkTMean-m0Temperature of APEC, mean (logkT_Mean_m0)phys.temperaturedoublelogkTStd-m0Temperature of APEC, standard deviation (logkT_Std_m0)phys.temperaturedoublelogAbundMedAbundance of the APEC model, median (logAbundanc_Med)phys.abunddoubleb_logAbundAbundance of the APEC model, 1sigma percentile lower limit (logAbundanc_Lo)phys.abunddoubleB_logAbundAbundance of the APEC model, 1sigma percentile upper limit (logAbundanc_Up)phys.abunddoublelogAbundMeanAbundance of the APEC model, mean (logAbundanc_Mean)phys.abunddoublelogAbundStdAbundance of the APEC model, standard deviation (logAbundanc_Std)phys.abunddoublelogApecNMedAPEC normalization, median (logApecNorm_Med)stat.fit.paramdoubleb_logApecNAPEC normalization, 1sigma percentile lower limit (logApecNorm_Lo)stat.fit.paramdoubleB_logApecNAPEC normalization, 1sigma percentile upper limit (logApecNorm_Up)stat.fit.paramdoublelogApecNMeanAPEC normalization, mean (logApecNorm_Mean)stat.fit.paramdoublelogApecNStdAPEC normalization, standard deviation (logApecNorm_Std)stat.fit.paramdoublelogBkgNMed-m0Background normalization, APEC normalization, median (logBkgNorm_Med_m0)stat.fit.paramdoubleb_logBkgN-m0Background normalization, 1sigma percentile lower limit (logBkgNorm_Lo_m0)stat.fit.paramdoubleB_logBkgN-m0Background normalization, 1sigma percentile upper limit (logBkgNorm_Up_m0)stat.fit.paramdoublelogBkgNMean-m0Background normalization, mean (logBkgNorm_Mean_m0)stat.fit.paramdoublelogBkgNStd-m0Background normalization, standard deviation (logBkgNorm_Std_m0)stat.fit.paramdoublelogZ-m0Bayesian evidence of model 0 (logZ_m0)stat.fit.paramdoubleRate-0.2-2.30.2-2.3keV source count rate (Rate_d2_2d3)ct/sphot.count;em.X-raydoubleDESdegSDSS declination (J2000) (SDSS_DEC)degpos.eq.dece_Rate-0.2-2.30.2-2.3keV source count rate error (RateErr_d2_2d3)ct/sstat.errordoubleRate-0.2-0.50.2-0.5keV source count rate (Rate_d2_d5)ct/sphot.count;em.X-raydoublee_Rate-0.2-0.50.2-0.5keV source count rate error (RateErr_d2_d5)ct/sstat.errordoubleRate-0.5-10.5-1keV source count rate (Rate_d5_1)ct/sphot.count;em.X-raydoublee_Rate-0.5-10.5-1keV source count rate error (RateErr_d5_1)ct/sstat.errordoubleRate-1-21-2keV source count rate (Rate_1_2)ct/sphot.count;em.X-raydoublee_Rate-1-21-2keV source count rate error (RateErr_1_2)ct/sstat.errordoubleRate-2-4.52-4.5keV source count rate (Rate_2_4d5)ct/sphot.count;em.X-raydoublee_Rate-2-4.52-4.5keV source count rate error (RateErr_2_4d5)ct/sstat.errordoubleRate-2.3-52.3-5keV source count rate (Rate_2d3_5)ct/sphot.count;em.X-raydoublee_Rate-2.3-52.3-5keV source count rate error (RateErr_2d3_5)ct/sstat.errordoubleRate-5-85-8keV source count rate (Rate_5_8)ct/sphot.count;em.X-raydoublee_Rate-5-85-8keV source count rate error (RateErr_5_8)ct/sstat.errordoubleExposureExposure time (Exposure)stime.duration;obs.exposuredoubleBkgCts_0.2-0.60.2-0.6keV background counts (BkgCts_d2_d6)ctinstr.background;em.X-ray.softfloate_BkgCts_0.2-0.60.2-0.6keV background counts error (BkgCtsErr_d2_d6)ctstat.errordoubleBkgCts-0.6-2.30.6-2.3keV background counts (BkgCts_d6_2d3)ctinstr.background;em.X-ray.softfloate_BkgCts-0.6-2.30.6-2.3keV background counts error (BkgCtsErr_d6_2d3)ctstat.errordoubleBkgCts-2.3-52.3-5keV background counts (BkgCts_2d3_5)ctinstr.background;em.X-ray.mediumfloate_BkgCts-2.3-52.3-5keV background counts error (BkgCtsErr_2d3_5)ctstat.errordoubleBkgCts-5-85-8keV background counts (BkgCts_5_8)ctinstr.background;em.X-ray.mediumfloate_BkgCts-5-85-8keV background counts error (BkgCtsErr_5_8)ctstat.errordoubleSrcCts0.5-2keV net counts calculated from the spectra (SrcCts)phot.count;arith.ratiodoublelogLintBF-s? rest-frame 0.5-2keV luminosity, best-fit model, selected Model (LumiIntr_BF_s)log(1e-07W)phys.luminositydoublenullablelogLintMed-s? rest-frame 0.5-2keV luminosity, median, selected Model (LumiIntr_Med_s)log(1e-07W)phys.luminositydoublenullableb_logLint-s? rest-frame 0.5-2keV luminosity, 1sigma lower limit, selected Model (LumiIntr_Lo1_s)log(1e-07W)phys.luminosity;em.X-raydoublenullableB_logLint-s? rest-frame 0.5-2keV luminosity, 1sigma upper limit, selected Model (LumiIntr_Up1_s)log(1e-07W)phys.luminosity;em.X-raydoublenullableb2_logLint-s? rest-frame 0.5-2keV luminosity, 2sigma lower limit, selected Model (LumiIntr_Lo2_s)log(1e-07W)phys.luminosity;em.X-raydoublenullableB2_logLint-s? rest-frame 0.5-2keV luminosity, 2sigma upper limit, selected Model (LumiIntr_Up2_s)log(1e-07W)phys.luminosity;em.X-raydoublenullablelogLintBF-h? rest-frame 2-10keV luminosity, best-fit model, selected Model (LumiIntr_BF_h)log(1e-07W)phys.luminositydoublenullableb_logLint-h? rest-frame 2-10keV luminosity, 1sigma lower limit, selected Model (LumiIntr_Lo1_h)log(1e-07W)phys.luminosity;em.X-raydoublenullableB_logLint-h? rest-frame 2-10keV luminosity, 1sigma upper limit, selected Model (LumiIntr_Up1_h)log(1e-07W)phys.luminosity;em.X-raydoublenullableb2_logLint-h? rest-frame 2-10keV luminosity, 2sigma lower limit, selected Model (LumiIntr_Lo2_h)log(1e-07W)phys.luminosity;em.X-raydoublenullableB2_logLint-h? rest-frame 2-10keV luminosity, 2sigma upper limit, selected Model (LumiIntr_Up2_h)log(1e-07W)phys.luminosity;em.X-raydoublenullablelogLintBF-2keV? Rest-frame 1.999-2.001keV luminosity, best-fit model, selected Mode (LumiIntr_BF_2keV)log(1e-07W)phys.luminositydoublenullablelogLintMed-2keV? Rest-frame 1.999-2.001keV luminosity, median, selected Model (LumiIntr_Med_2keV)log(1e-07W)phys.luminositydoublenullableb_logLint-2keV? Rest-frame 1.999-2.001keV luminosity, 1sigma lower limit, selected (LumiIntr_Lo1_2keV)log(1e-07W)phys.luminosity;em.X-raydoublenullableB_logLint-2keV? Rest-frame 1.999-2.001keV luminosity, 1sigma upper limit, selected (LumiIntr_Up1_2keV)log(1e-07W)phys.luminosity;em.X-raydoublenullableb2_logLint-2keV? Rest-frame 1.999-2.001keV luminosity, 2sigma lower limit, selected (LumiIntr_Lo2_2keV)log(1e-07W)phys.luminosity;em.X-raydoublenullableB2_logLint-2keV? Rest-frame 1.999-2.001keV luminosity, 2sigma upper limit, selected (LumiIntr_Up2_2keV)log(1e-07W)phys.luminosity;em.X-raydoublenullableLxModelThe chosen model for luminosity measurement (LxModel)meta.id;stat.fitintMJDMJD (MJD)time.epochintFiberIdFiber ID (FIBERID)meta.idintCatalogIdCatalog ID (CATALOGID)meta.id;meta.tableRASdegSDSS right ascension (J2000) (SDSS_RA)degpos.eq.ralogL13501350{AA} luminosity (LogL1350)log(1e-07W)phys.luminositydoublee_logL1350? 1350{AA} luminosity error (LogL1350_err)log(1e-07W)stat.errordoublenullablelogL30003000{AA} luminosity (LogL3000)log(1e-07W)phys.luminositydoublee_logL3000? 3000{AA} luminosity error (LogL3000_err)log(1e-07W)stat.errordoublenullablelogL51005100{AA} luminosity (LogL5100)log(1e-07W)phys.luminositydoublee_logL5100? 5100{AA} luminosity error (LogL5100_err)log(1e-07W)stat.errordoublenullablelogMBHHbetaBlack hole mass based on Hbeta (logMBH_Hbeta)log(solMass)phys.massdoublee_logMBHHbeta? Black hole mass error based on Hbeta (logMBH_Hbeta_err)log(solMass)stat.errordoublenullablelogMBHMgIIBlack hole mass based on MgII (logMBH_MgII)log(solMass)phys.massdoublee_logMBHMgII? Black hole mass error based on MgII (logMBH_MgII_err)log(solMass)stat.errordoublenullablelogMBHCIVBlack hole mass based on CIV (logMBH_CIV)log(solMass)phys.massdoublee_logMBHCIV? Black hole mass error based on CIV (logMBH_CIV_err)log(solMass)stat.errordoublenullableHa-br-fluxHalpha flux (Ha_br_flux)mW.m**-2phot.flux;em.line.HalphadoubleHa-br-LogLHalpha luminosity (Ha_br_LogL)1e-07Wphys.luminosity;em.line.Halphadoublee_Ha-br-LogL? Halpha luminosity error (Ha_br_LogL_err)1e-07Wstat.errordoublenullableHa-br-FWHMHalpha FWHM (Ha_br_FWHM)km/sphys.angSizedoublee_Ha-br-FWHM? Halpha FWHM error (Ha_br_FWHM_err)km/sphys.angSizedoublenullableHb-br-fluxHbeta flux (Hb_br_flux)mW.m**-2phot.flux;em.line.Hbetadoublee_Hb-br-flux? Hbeta flux error (Hb_br_flux_err)mW.m**-2stat.error;phot.fluxdoublenullableHb-br-LogLHbeta luminosity (Hb_br_LogL)1e-07Wphys.luminosity;em.line.Hbetadoublee_Hb-br-LogL? Hbeta luminosity error (Hb_br_LogL_err)1e-07Wstat.errordoublenullableHb-br-FWHMHbeta FWHM (Hb_br_FWHM)km/sphys.angSizedoublee_Hb-br-FWHM? Hbeta FWHM error (Hb_br_FWHM_err)km/sphys.angSizedoublenullableMgII-br-fluxMgII flux (MgII_br_flux)mW.m**-2phot.fluxdoublee_MgII-br-flux? MgII flux error (MgII_br_flux_err)mW.m**-2stat.error;phot.fluxdoublenullableMgII-br-LogLMgII luminosity (MgII_br_LogL)1e-07Wphys.luminositydoublee_MgII-br-LogL? MgII luminosity error (MgII_br_LogL_err)1e-07Wstat.errordoublenullableMgII-br-FWHMMgII FWHM (MgII_br_FWHM)km/sphys.angSizedoublee_MgII-br-FWHM? MgII FWHM error (MgII_br_FWHM_err)km/sphys.angSizedoublenullableCIV-br-fluxCIV flux (CIV_br_flux)mW.m**-2phot.fluxdoublee_CIV-br-flux? CIV flux error (CIV_br_flux_err)mW.m**-2stat.error;phot.fluxdoublenullableCIV-br-LogLCIV luminosity (CIV_br_LogL)1e-07Wphys.luminositydoublee_CIV-br-LogL? CIV luminosity error (CIV_br_LogL_err)1e-07Wstat.errordoublenullableCIV-br-FWHMCIV FWHM (CIV_br_FWHM)km/sphys.angSizedoublee_CIV-br-FWHM? CIV FWHM error (CIV_br_FWHM_err)km/sphys.angSizedoublenullableLbolBolometric luminosity (Lbol)1e-07Wphys.luminositydoublee_LbolBolometric luminosity error (Lbol_err)1e-07Wstat.errordoublelogMBH? Adopted black hole mass (logMBH)log(solMass)phys.massdoublenullablee_logMBHAdopted black hole mass error (logMBH_err)log(solMass)stat.errordoubleLedd? Eddington luminosity (Ledd)phys.luminosity;arith.ratiodoublenullablee_LeddEddington luminosity error (Ledd_err)stat.errordoubleGoodMBH[0/1] whether the black hole mass is good (GoodMBH)meta.codedoubleNameeROSITA source Name (Name) (1)meta.id;meta.maincharSDSS-DR[DR17/DR18] SDSS DR version (SDSS_DR)meta.softwarechar