J/A+A/661/A5ivo://CDS.VizieR/J/A+A/661/A5doi:10.26093/cds/vizier.36610005CDSLiu T.Buchner J.Nandra K.Merloni A.Dwelly T.Sanders J.S.,Salvato M.Arcodia R.Brusa M.Wolf J.Georgakakis A.Boller T.,Krumpe M.Lamer G.Waddell S.Urrutia T.Schwope A.Robrade J.,Wilms J.Dauser T.Comparat J.Toba Y.Ichikawa K.Iwasawa K.,Shen Y.Medel H.I.2026-06-11T20:02:29Z2022-05-18T13:13:25ZCDS support team

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

cds-question@unistra.frsurveysx-ray-sourcesquasarsactive-galactic-nucleiThe eROSITA Final Equatorial Depth Survey (eFEDS), observed with eROSITA ahead of its planned four-year all-sky survey, is the largest contiguous-field X-ray survey at present. It yielded a large sample of X-ray sources with very rich multiband photometric and spectroscopic coverage. We present here the eFEDS active galactic nuclei (AGN) catalog and the eROSITA X-ray spectral properties of the eFEDS sources. Using a Bayesian method, we performed a systematic X-ray spectral analysis for all the eFEDS sources. We adopted multiple spectral models, including single-component power-law or hot-plasma models and double-component models of a power law plus soft excess. We investigated the capacity of eROSITA X-ray spectra for constraining AGN spectral shapes through a detailed analysis of the posterior parameter probability distribution functions. Hierarchical Bayesian modeling (HBM) was used to recover the spectral parameter distribution of the sample. The source fluxes and luminosities were measured from the posterior of the spectral fitting. The eFEDS AGN catalog (22079 sources) comprises ~80% of the eFEDS point sources. Despite a large number of faint sources, our spectral fitting provides reasonable measurements of spectral shapes and intrinsic luminosities for a majority of the sources. Because of sample selection bias, this AGN catalog is dominated by X-ray unobscured sources, with an obscured (logNH>21.5) fraction of 8%; the power-law emission of the hot corona is also relatively soft, with a typical slope of 2.0. For type-I AGN, the X-ray emission is well correlated with the UV emission with the usual anticorrelation between the X-ray to UV spectral slope alpha_OX and the UV luminosity. The X-ray spectral properties measured with various models are presented for all the eFEDS sources.2022A&A...661A...5Lhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/661/A5CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toJ/A+A/661/A1 : The eFEDS X-ray catalogs (V7.4) (Brunner+, 2022)J/A+A/661/A2 : Galaxy clusters and groups in eFEDS (Liu+, 2022)J/A+A/661/A3 : eFEDS counterparts to point-like sources (Salvato+, 2022)J/A+A/661/A4 : eFEDS optical cluster and group catalog (Klein+, 2022)J/A+A/661/A7 : X-ray properties of eFEDS clusters and groups (Bahar+, 2022)J/A+A/661/A8 : eFEDS catalogue of variable X-ray sources (Boller+, 2022)J/A+A/661/A10 : eFEDS galaxy clusters and groups in disguise (Bulbul+, 2022)J/A+A/661/A23 : Exoplanet X-ray irradiation & evaporation rates (Foster+, 2022)J/A+A/661/A24 : Corona-chromosphere connection (Fuhrmeister+, 2022)J/A+A/661/A29 : First eROSITA study of nearby M dwarfs (Magaudda+, 2022)J/A+A/661/A34 : eta Cha cluster eROSITA X-ray scan (Robrade+, 2022)J/A+A/661/A35 : eROSITA study of 47 Tuc globular cluster (Saeedi+, 2022)J/A+A/661/A38 : SRG/ART-XC 1st year all-sky X-ray survey (Pavlinsky+, 2022)J/A+A/661/A40 : eRASS1 X-ray sources Sco-Cen members (Schmitt+, 2022)J/A+A/661/A44 : A first eROSITA view of ultracool dwarfs (Stelzer+, 2022)https://erosita.mpe.mpg.de/edr/eROSITAObservations/Catalogues/liuT/eFEDS_AGN_spec_V9.html : Home Pagehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/661/A5https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/661/A5http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/661/A5https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/661/A5https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/661/A5http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/661/A5GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/A+A/661/A5/table1 (The eFEDS AGN catalog)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/661/A5/table1?https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/661/A5/table1?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/661/A5/table1?GETtext/xml+votable180.050000true144.25383285520851.09592040906240.005555555555555556Cone search capability for table J/A+A/661/A5/table2 (Spectral properties)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/661/A5/table2?https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/661/A5/table2?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/661/A5/table2?GETtext/xml+votable180.050000true144.2538911.10.0055555555555555564/256 1365 1367 1706-1707 5/1028-1030 1032-1034 5457 5459 5464-5465 5493 6818-6820 6822-6823 6834 6840-6842 10238-10239 6/4124-4126 4140-4141 4144 4146 4160-4161 4224 4226 21827 21833-21835 21868-21869 21969 27183 27194 27269-27271 27286-27287 27342-27343 27372 27374 40947 40949-409513.830199579824256e-20 6.513807192489934e-20https://cdsarc.cds.unistra.fr/viz-bin/moc/J/A+A/661/A5?format=asciiX-raydefaultJ/A+A/661/A5/table1The eFEDS AGN catalogrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintID-SRC[1/32683] ID of the sources in the eFEDS main X-ray catalog (Paper I) (ID_SRC)meta.id;meta.maininte_W1mag? LS8-WISE W1 magnitude error (Paper II) (W1_ERR)magstat.error;phot.magdoublenullableW2mag? LS8-WISE W2 AB magnitude (Paper II) (W2)magphot.mag;em.IR.4-8umdoublenullablee_W2mag? LS8-WISE W2 magnitude error (Paper II) (W2_ERR)magstat.error;phot.magdoublenullablePaperIDisplay the Paper I (Brunner et al., Cat. J/A+A/661/A1) datameta.ref.urlcharRAc[126.24/145.59] Right ascension (J2000), astrometric corrected (Paper I) (RA_CORR)degpos.eq.ra;meta.mainindexedDEc[-2.91/5.97] Declination (J2000), astrometric corrected (Paper I) (DEC_CORR)degpos.eq.dec;meta.mainindexedDetLike0.2-2.3 keV source detection likelihood (Paper I) (DET_LIKE)stat.likelihooddoubleinArea90Whether located inside the inner 90%-area region of eFEDS (Paper I) (inArea90)meta.codedoubleRALdeg[126.23/145.59] Right ascension (J2000) of the best LS8 counterpart (Paper II) (CTP_LS8_RA)degpos.eq.raDELdeg[-2.91/5.97] Declination (J2000) of the best LS8 counterpart (Paper II) (CTP_LS8_DEC)degpos.eq.decCTPqual[2/4] Counterpart quality (Paper II) A value >=2 is recommended (CTP_quality)meta.code.qualintCTPClass[2/3] Classification of the optical counterpart (Paper II) (CTP_CLASS) (1)src.classintCTPz[0.0/8.0] Redshift of the optical counterpart (Paper II) (CTP_REDSHIFT)src.redshift.photdoubleCTPzgrade[2/5] Redshift Grade (Paper II) A value >=3 is recommended (CTP_REDSHIFT_GRADE)meta.code.qualintinKiDSFlag[0/1] Whether located inside the region of the KiDS survey (Paper II) (in_KiDS_flag)meta.codeintLxModel[1/5] Index of selected model for luminosity measurement (LxModel) (2)meta.codeintNHclass[1/4] Class of AGN NH measurement with model 1 (single-powerlaw) (NHclass) (3)meta.codeintFSModel[3/6] Index of selected model for 0.5-2keV flux (FSModel) (4)meta.codeintFHModel[5/7] Index of selected model for 2.3-5keV flux (FHModel) (5)meta.codeintgalNHTotal column density of Galactic absorption (galNH)cm**-2phys.columnDensitydoublegalNHIHI column density from HI4PI (galNHI)cm**-2phys.columnDensitydoubleSrcCtsSource net counts in the 0.2-5 keV band (SrcCts)ctphot.count;em.X-raydoubleFluxcMedSAbsorption corrected flux in observed 0.5-2 keV, posterior median (FluxCorr_Med_s)mW.m**-2phot.flux;em.X-raydoubleb_FluxcSAbsorption corrected flux in observed 0.5-2 keV, 1sigma lower limit (FluxCorr_Lo1_s)mW.m**-2phot.flux;em.X-ray.softdoubleB_FluxcSAbsorption corrected flux in observed 0.5-2 keV, 1sigma upper limit (FluxCorr_Up1_s)mW.m**-2phot.flux;em.X-ray.softdoubleFluxcMedTAbsorption corrected flux in observed 2.3-5 keV, posterior median (FluxCorr_Med_t)mW.m**-2phot.flux;em.X-raydoubleb_FluxcTAbsorption corrected flux in observed 2.3-5 keV, 1sigma lower limit (FluxCorr_Lo1_t)mW.m**-2phot.flux;em.X-ray.mediumdoubleB_FluxcTAbsorption corrected flux in observed 2.3-5 keV, 1sigma upper limit (FluxCorr_Up1_t)mW.m**-2phot.flux;em.X-ray.mediumdoubleFluxIMedSAbsorption corrected flux in rest-frame 0.5-2 keV, posterior median (FluxIntr_Med_s)mW.m**-2phot.flux;em.X-raydoubleb_FluxISAbsorption corrected flux in rest-frame 0.5-2keV, 1sigma lower limit (FluxIntr_Lo1_s)mW.m**-2phot.flux;em.X-ray.softdoubleB_FluxISAbsorption corrected flux in rest-frame 0.5-2keV, 1sigma upper limit (FluxIntr_Up1_s)mW.m**-2phot.flux;em.X-ray.softdoubleFluxIMed2keVAbsorption corrected flux at rest-frame 2keV, median (FluxIntr_Med_2keV)mW.m**-2.eV**-1phot.flux;em.X-raydoubleb_FluxI2keVAbsorption corrected flux at rest-frame 2keV, 1sigma lower limit (FluxIntr_Lo1_2keV)mW.m**-2.eV**-1phot.fluxdoubleB_FluxI2keVAbsorption corrected flux at rest-frame 2keV, 1sigma upper limit (FluxIntr_Up1_2keV)mW.m**-2.eV**-1phot.fluxdoubleLumIMedSIntrinsic luminosity in rest-frame 0.5-2 keV, posterior median (LumiIntr_Med_s)1e-07Wphys.luminosity;em.X-rayfloatb_LumISIntrinsic luminosity in rest-frame 0.5-2 keV, 1sigma lower limit (LumiIntr_Lo1_s)1e-07Wphys.luminosity;em.X-ray.softfloatB_LumISIntrinsic luminosity in rest-frame 0.5-2 keV, 1sigma upper limit (LumiIntr_Up1_s)1e-07Wphys.luminosity;em.X-ray.softfloatLumIMed2keVIntrinsic luminosity at rest-frame 2keV, posterior median in erg/s/eV (LumiIntr_Med_2keV)1e-07W.eV**-1phys.luminosity;em.X-raydoubleb_LumI2keVIntrinsic luminosity at rest-frame 2keV, 1sigma lower limit in erg/s/eV (LumiIntr_Lo1_2keV)1e-07W.eV**-1phys.luminositydoubleB_LumI2keVIntrinsic luminosity at rest-frame 2keV, 1sigma upper limit in erg/s/eV (LumiIntr_Up1_2keV)1e-07W.eV**-1phys.luminositydoubleFluxObsMedSObserved flux in observed 0.5-2 keV, posterior median (FluxObsv_Med_s)mW.m**-2phot.flux;em.X-raydoubleb_FluxObsSObserved flux in observed 0.5-2 keV, 1sigma lower limit (FluxObsv_Lo1_s)mW.m**-2phot.flux;em.X-ray.softdoubleB_FluxObsSObserved flux in observed 0.5-2 keV, 1sigma upper limit (FluxObsv_Up1_s)mW.m**-2phot.flux;em.X-ray.softdoubleFluxObsMedTObserved flux in observed 2.3-5 keV, posterior median (FluxObsv_Med_t)mW.m**-2phot.flux;em.X-raydoubleb_FluxObsTObserved flux in observed 2.3-5 keV, 1sigma lower limit (FluxObsv_Lo1_t)mW.m**-2phot.flux;em.X-ray.mediumdoubleB_FluxObsTObserved flux in observed 2.3-5 keV, 1sigma upper limit (FluxObsv_Up1_t)mW.m**-2phot.flux;em.X-ray.mediumdoublelognHKLm1log AGN column density, KL divergence (in nats units) (lognH_KL_m1)stat.fit.paramdoubleb_lognHm1log AGN column density, HDI lower limit (lognH_HLo_m1)log(cm**-2)phys.columnDensity;stat.mindoubleB_lognHm1log AGN column density, HDI upper limit (lognH_HUp_m1)log(cm**-2)phys.columnDensity;stat.maxdoublelognHMedm1log AGN column density, posterior median (lognH_Med_m1)log(cm**-2)phys.columnDensitydoubleGammaKLm3primary power-law slope in model 3, KL divergence (in nats units) (Gamma_KL_m3)stat.fit.paramdoubleb_GammaHm3primary power-law slope in model 3, HDI lower limit (Gamma_HLo_m3)arith.grad;stat.param;meta.modelleddoubleB_GammaHm3primary power-law slope in model 3, HDI upper limit (Gamma_HUp_m3)arith.grad;stat.param;meta.modelleddoubleGammaMedm3primary power-law slope in model 3, posterior median (Gamma_Med_m3)spect.indexdoublelogZm0log Bayesian evidence with model 0: APEC (logZ_m0)stat.fit.paramdoublelogZm1log Bayesian evidence with model 1: single powerlaw (logZ_m1)stat.fit.paramdoublelogZm2log Bayesian evidence with model 2: double powerlaw (logZ_m2)stat.fit.paramdoublelogZm3log Bayesian evidence with model 3: powerlaw + blackbody (logZ_m3)stat.fit.paramdoublelogZm4log Bayesian evidence with model 4: powerlaw with Gamma fixed at 2.0 (logZ_m4)stat.fit.paramdoublelogZm5log Bayesian evidence with model 5: shape-fixed powerlaw (logZ_m5)stat.fit.paramdoubleL2500? The rest-frame 2500 luminosity in erg/s/Hz (L2500)1e-07W.Hz**-1phys.luminositydoublenullableL5100? The rest-frame 5100 luminosity in erg/s/Hz (L5100)1e-07W.Hz**-1phys.luminositydoublenullableW1mag? LS8-WISE W1 AB magnitude (Paper II) (W1)magphot.mag;em.IR.3-4umdoublenullablePaperIIDisplay the Paper II (Salvato et al., Cat. J/A+A/661/A3) datameta.ref.urlcharCTPLS8ID of the best LS8 counterpart (Paper II) (CTP_LS8_UNIQUE_OBJID)meta.idcharJ/A+A/661/A5/table2Spectral propertiese_Rate1-2Net count rate error in 1-2 keV (RateErr_1_2)ct/sstat.errordoubleRate2-4.5Net count rate in 2-4.5 keV (Rate_2_4d5)ct/sphot.count;em.X-raydoublee_Rate2-4.5Net count rate error in 2-4.5 keV (RateErr_2_4d5)ct/sstat.errordoublerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintID-SRC[1/32683] ID of the sources in the eFEDS main X-ray catalog (Paper I) (ID_SRC)meta.id;meta.mainintRAcdeg[126.24/145.66] Right ascension (J2000), astrometric corrected (Paper I) (RA_CORR)degpos.eq.raDEcdeg[-2.91/5.97] Declination (J2000), astrometric corrected (Paper I) (DEC_CORR)degpos.eq.decDetLike[6.0/33254.59] 0.2-2.3 keV source detection likelihood (Paper I) (DET_LIKE)stat.likelihooddoubleExtLikeX-ray source extent likelihood (Paper I) (EXT_LIKE)stat.likelihooddoubleinArea90Whether located inside the inner 90%-area region of eFEDS (Paper I) (inArea90)meta.codedoublegalNHTotal column density of Galactic absorption (galNH)cm**-2physdoublegalNHIHI column density from HI4PI (galNHI)cm**-2phys.columnDensitydoubleExpTimeSpectra exposure time (Exposure)stime.duration;obs.exposuredoubleSrcCtsSource net counts in the 0.2-5 keV band (SrcCts)ctphot.count;em.X-raydoubleRAJ2000[126.24/145.66] Right ascension (J2000) before astrometric correction (Paper I) (RA)degpos.eq.ra;meta.mainindexedDEJ2000[-2.91/5.97] Declination (J2000) before astrometric correction (Paper I) (DEC)degpos.eq.dec;meta.mainindexedRad[12/259] Source extraction radius (Rad)arcsecphys.angSizeintAnn1[22/515] Inner radius of background extraction region (Ann1)arcsecphys.angSize;obs.fieldintAnn2[171/900] Outer radius of background extraction region (Ann2)arcsecphys.angSize;obs.fieldintRegAreaGeometry area of source extraction region (REGAREA_s)deg**2phys.angSizedoubleBackscalSource BACKSCAL (Backscal_s)deg**2phys.angSizedoubleBackscalBkgBackground BACKSCAL (Backscal_b)deg**2phys.angSizedoubleFSModel[0/6] Index of selected model for 0.5-2keV flux (FSModel) (1)meta.codeintFHModel[5/7] Index of selected model for 2.3-5keV flux (FHModel) (2)meta.codeintRate0.2-2.3Net count rate in 0.2-2.3 keV (Rate_d2_2d3)ct/sphot.count;em.X-raydoublee_Rate0.2-2.3Net count rate error in 0.2-2.3 keV (RateErr_d2_2d3)ct/sstat.errordoubleRate0.2-0.5Net count rate in 0.2-0.5 keV (Rate_d2_d5)ct/sphot.count;em.X-raydoublee_Rate0.2-0.5Net count rate error in 0.2-0.5 keV (RateErr_d2_d5)ct/sstat.errordoubleRate0.5-1Net count rate in 0.5-1 keV (Rate_d5_1)ct/sphot.count;em.X-raydoublee_Rate0.5-1Net count rate error in 0.5-1 keV (RateErr_d5_1)ct/sstat.errordoubleRate1-2Net count rate in 1-2 keV (Rate_1_2)ct/sphot.count;em.X-raydoubleRate2.3-5Net count rate in 2.3-5 keV (Rate_2d3_5)ct/sphot.count;em.X-raydoublee_Rate2.3-5Net count rate error in 2.3-5 keV (RateErr_2d3_5)ct/sstat.errordoubleRate5-8Net count rate in 5-8 keV (Rate_5_8)ct/sphot.count;em.X-raydoublee_Rate5-8Net count rate error in 5-8 keV (RateErr_5_8)ct/sstat.errordoubleBkgCts0.2-0.6Background counts in 0.2-0.6 keV (BkgCts_d2_d6)ctinstr.background;em.X-ray.softfloate_BkgCts0.2-0.6Background counts error in 0.2-0.6 keV (BkgCtsErr_d2_d6)ctstat.errordoubleBkgCts0.6-2.3Background counts in 0.6-2.3 keV (BkgCts_d6_2d3)ctinstr.background;em.X-ray.softfloate_BkgCts0.6-2.3Background counts error in 0.6-2.3 keV (BkgCtsErr_d6_2d3)ctstat.errordoubleBkgCts2.3-5Background counts in 2.3-5 keV (BkgCts_2d3_5)ctinstr.background;em.X-ray.mediumfloate_BkgCts2.3-5Background counts error in 2.3-5 keV (BkgCtsErr_2d3_5)ctstat.errordoubleBkgCts5-8Background counts in 5-8 keV (BkgCts_5_8)ctinstr.background;em.X-ray.mediumfloate_BkgCts5-8Background counts error in 5-8 keV (BkgCtsErr_5_8)ctstat.errordoublePSFCor0.2-0.5PSF-loss correction (ARF CORRPSF) averaged in 0.2-0.5 keV (PSFCor_d2_d5)arith.factordoublePSFCor0.5-1PSF-loss correction (ARF CORRPSF) averaged in 0.5-1 keV (PSFCor_d5_1)arith.factordoublePSFCor1-2PSF-loss correction (ARF CORRPSF) averaged in 1-2 keV (PSFCor_1_2)arith.factordoublePSFCor2.3-5PSF-loss correction (ARF CORRPSF) averaged in 2.3-5 keV (PSFCor_2d3_5)arith.factordoubleNempty[35/771] Number of empty channels between channel 20 and 900 (Nempty)meta.numberintFluxObsMedSObserved flux in observed 0.5-2 keV, posterior median (FluxObsv_Med_s)mW.m**-2phot.flux;em.X-raydoubleb_FluxObsSObserved flux in observed 0.5-2 keV, 1sigma lower limit (FluxObsv_Lo1_s)mW.m**-2phot.flux;em.X-ray.softdoubleB_FluxObsSObserved flux in observed 0.5-2 keV, 1sigma upper limit (FluxObsv_Up1_s)mW.m**-2phot.flux;em.X-ray.softdoubleFluxObsMedTObserved flux in observed 2.3-5 keV, posterior median (FluxObsv_Med_t)mW.m**-2phot.flux;em.X-raydoubleb_FluxObsTObserved flux in observed 2.3-5 keV, 1sigma lower limit (FluxObsv_Lo1_t)mW.m**-2phot.flux;em.X-ray.mediumdoubleB_FluxObsTObserved flux in observed 2.3-5 keV, 1sigma upper limit (FluxObsv_Up1_t)mW.m**-2phot.flux;em.X-ray.mediumdoublePaperIDisplay the Paper I (Brunner et al., Cat. J/A+A/661/A1) datameta.ref.urlcharPaperIIDisplay the Paper II (Salvato et al., Cat. J/A+A/661/A3) datameta.ref.urlcharJ/A+A/661/A5/table3APEC fitting resultslogkTMeanlog temperature, mean (logkT_Mean)log(keV)phys.temperaturedoubles_logkTlog temperature, standard deviation (logkT_Std)log(keV)stat.stdev;phys.temperaturedoublelogAbundMedlog abundance, posterior median (logAbundanc_Med)phys.abunddoublerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintID-SRC[1/32683] ID of the sources in the eFEDS main X-ray catalog (Paper I) (ID_SRC)meta.id;meta.mainintzThe redshift adopted for the spectral model (Redshift)src.redshiftfloatlognHKLlog AGN column density, KL divergence (in nats units) (lognH_KL)stat.fit.paramdoubleb_lognHHlog AGN column density, HDI lower limit (lognH_HLo)log(cm**-2)phys.columnDensity;stat.mindoubleB_lognHHlog AGN column density, HDI upper limit (lognH_HUp)log(cm**-2)phys.columnDensity;stat.maxdoublelogkTKLlog temperature, KL divergence (in nats units) (logkT_KL)stat.fit.paramdoubleb_logkTHlog temperature, HDI lower limit (logkT_HLo)log(keV)phys.temperature;stat.mindoubleB_logkTHlog temperature, HDI upper limit (logkT_HUp)log(keV)phys.temperature;stat.maxdoublelogAbundKLlog abundance, KL divergence (in nats units) (logAbundanc_KL)stat.fit.paramdoubleb_logAbunHlog abundance, HDI lower limit (logAbundanc_HLo)meta.notedoubleB_logAbunHlog abundance, HDI upper limit (logAbundanc_HUp)meta.notedoublelogApecNormKLlog APEC normalization, KL divergence (in nats units) (logApecNorm_KL)stat.fit.paramdoubleb_logApecNormHlog APEC normalization, HDI lower limit (logApecNorm_HLo)log(cm**-5)arith.zp;stat.mindoubleB_logApecNormHlog APEC normalization, HDI upper limit (logApecNorm_HUp)log(cm**-5)arith.zp;stat.maxdoublelognHBFlog AGN column density, best-fit model (lognH_BF)log(cm**-2)phys.columnDensitydoublelogkTBFlog temperature, best-fit model (logkT_BF)log(keV)phys.temperaturedoublelogAbundBFlog abundance, best-fit model (logAbundanc_BF)phys.abunddoublelogApecNBFlog APEC normalization, best-fit model (logApecNorm_BF)log(cm**-5)stat.fit.paramdoubleFluxObsBFSObserved flux in observed 0.5-2 keV, best-fit model (FluxObsv_BF_s)mW.m**-2phot.flux;em.X-raydoubleFluxObsMedSObserved flux in observed 0.5-2 keV, posterior median (FluxObsv_Med_s)mW.m**-2phot.flux;em.X-raydoubleb_FluxObsSObserved flux in observed 0.5-2 keV, 1sigma lower limit (FluxObsv_Lo1_s)mW.m**-2phot.flux;em.X-ray.softdoubleB_FluxObsSObserved flux in observed 0.5-2 keV, 1sigma upper limit (FluxObsv_Up1_s)mW.m**-2phot.flux;em.X-ray.softdoubleb2_FluxObsSObserved flux in observed 0.5-2 keV, 2sigma lower limit (FluxObsv_Lo2_s)mW.m**-2phot.flux;em.X-raydoubleB2_FluxObsSObserved flux in observed 0.5-2 keV, 2sigma upper limit (FluxObsv_Up2_s)mW.m**-2phot.flux;em.X-raydoubleFluxObsBFTObserved flux in observed 2.3-5 keV, best-fit model (FluxObsv_BF_t)mW.m**-2phot.flux;em.X-raydoubleFluxObsMedTObserved flux in observed 2.3-5 keV, posterior median (FluxObsv_Med_t)mW.m**-2phot.flux;em.X-raydoubleb_FluxObsTObserved flux in observed 2.3-5 keV, 1sigma lower limit (FluxObsv_Lo1_t)mW.m**-2phot.flux;em.X-ray.mediumdoubleB_FluxObsTObserved flux in observed 2.3-5 keV, 1sigma upper limit (FluxObsv_Up1_t)mW.m**-2phot.flux;em.X-ray.mediumdoubleb2_FluxObsTObserved flux in observed 2.3-5 keV, 2sigma lower limit (FluxObsv_Lo2_t)mW.m**-2phot.flux;em.X-raydoubleB2_FluxObsTObserved flux in observed 2.3-5 keV, 2sigma upper limit (FluxObsv_Up2_t)mW.m**-2phot.flux;em.X-raydoublelognHMedlog AGN column density, posterior median (lognH_Med)log(cm**-2)phys.columnDensitydoubleb_lognHlog AGN column density, percentile lower limit (lognH_Lo)log(cm**-2)phys.columnDensity;stat.mindoubleB_lognHlog AGN column density, percentile upper limit (lognH_Up)log(cm**-2)phys.columnDensity;stat.maxdoublelognHMeanlog AGN column density, mean (lognH_Mean)log(cm**-2)phys.columnDensitydoubles_lognHlog AGN column density, standard deviation (lognH_Std)log(cm**-2)stat.stdev;phys.columnDensitydoublelogkTMedlog temperature, posterior median (logkT_Med)log(keV)phys.temperaturedoubleb_logkTlog temperature, percentile lower limit (logkT_Lo)log(keV)phys.temperature;stat.mindoubleB_logkTlog temperature, percentile upper limit (logkT_Up)log(keV)phys.temperature;stat.maxdoubleb_logAbundlog abundance, percentile lower limit (logAbundanc_Lo)meta.notedoubleB_logAbundlog abundance, percentile upper limit (logAbundanc_Up)meta.notedoublelogAbundMeanlog abundance, mean (logAbundanc_Mean)phys.abunddoubles_logAbundlog abundance, standard deviation (logAbundanc_Std)stat.stdevdoublelogApecNMedlog APEC normalization, posterior median (logApecNorm_Med)log(cm**-5)stat.fit.paramdoubleb_logApecNlog APEC normalization, percentile lower limit (logApecNorm_Lo)log(cm**-5)arith.zp;stat.mindoubleB_logApecNlog APEC normalization, percentile upper limit (logApecNorm_Up)log(cm**-5)arith.zp;stat.maxdoublelogApecNMeanlog APEC normalization, mean (logApecNorm_Mean)log(cm**-5)stat.fit.paramdoubles_logApecNlog APEC normalization, standard deviation (logApecNorm_Std)log(cm**-5)stat.stdev;arith.zp;arith.ratiodoublelogBkgNMedlog background normalization, posterior median (logBkgNorm_Med)instr.backgrounddoubleb_logBkgNlog background normalization, percentile lower limit (logBkgNorm_Lo)instr.background;arith.ratiodoubleB_logBkgNlog background normalization, percentile upper limit (logBkgNorm_Up)instr.background;arith.ratiodoublelogBkgNMeanlog background normalization, mean (logBkgNorm_Mean)instr.backgrounddoubles_logBkgNlog background normalization, standard deviation (logBkgNorm_Std)instr.background;arith.ratiodoublechi25? Chi^2 of the best-fit model against the rebinned data (>=25 cts/bin) (chi25)stat.fit.chi2doublenullabledof25? DOF of the rebinned data, which has at least 25 counts per bin (dof25)stat.fit.dofintnullablelogZlog10 Bayesian evidence (logZ)stat.fit.paramdoublePaperIDisplay the Paper I (Brunner et al., Cat. J/A+A/661/A1) datameta.ref.urlcharPaperIIDisplay the Paper II (Salvato et al., Cat. J/A+A/661/A3) datameta.ref.urlcharJ/A+A/661/A5/table4Single-powerlaw resultsB_FluxISAbsorption corrected flux in rest-frame 0.5-2keV, 1sigma upper limit (FluxIntr_Up1_s)mW.m**-2phot.flux;em.X-ray.softdoubles_lognHlog AGN column density, standard deviation (lognH_Std)log(cm**-2)stat.stdev;phys.columnDensitydoublelogPowNMedlog power-law normalization, posterior median (logPowNorm_Med)ph.keV**-1.cm**-2.s**-1stat.fit.paramdoublerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintID-SRC[1/32683] ID of the sources in the eFEDS main X-ray catalog (Paper I) (ID_SRC)meta.id;meta.mainintz[-0.01/8.0] The redshift adopted for the spectral model (Redshift)src.redshiftdoubleGammaKLpower-law slope, KL divergence (in nats units) (Gamma_KL)stat.fit.paramdoubleb_GammaHpower-law slope, HDI lower limit (Gamma_HLo)arith.grad;stat.mindoubleB_GammaHpower-law slope, HDI upper limit (Gamma_HUp)arith.grad;stat.maxdoublelognHKLlog AGN column density, KL divergence (in nats units) (lognH_KL)stat.fit.paramdoubleb_lognHHlog AGN column density, HDI lower limit (lognH_HLo)log(cm**-2)phys.columnDensity;stat.mindoubleB_lognHHlog AGN column density, HDI upper limit (lognH_HUp)log(cm**-2)phys.columnDensity;stat.maxdoublelogPowNKLlog power-law normalization, KL divergence (in nats units) (logPowNorm_KL)stat.fit.paramdoubleb_logPowNHlog power-law normalization, HDI lower limit (logPowNorm_HLo)ph.keV**-1.cm**-2.s**-1arith.zp;arith.ratiodoubleB_logPowNHlog power-law normalization, HDI upper limit (logPowNorm_HUp)ph.keV**-1.cm**-2.s**-1arith.zp;arith.ratiodoubleGammaBFpower-law slope, best-fit model (Gamma_BF)spect.indexdoublelognHBFlog AGN column density, best-fit model (lognH_BF)log(cm**-2)phys.columnDensity;meta.modelleddoublelogPowNBFlog power-law normalization, best-fit model (logPowNorm_BF)ph.keV**-1.cm**-2.s**-1stat.fit.paramdoubleFluxObsBFSObserved flux in observed 0.5-2 keV, best-fit model (FluxObsv_BF_s)mW.m**-2phot.flux;em.X-raydoubleFluxObsMedSObserved flux in observed 0.5-2 keV, posterior median (FluxObsv_Med_s)mW.m**-2phot.flux;em.X-raydoubleb_FluxObsSObserved flux in observed 0.5-2 keV, 1sigma lower limit (FluxObsv_Lo1_s)mW.m**-2phot.flux;em.X-ray.softdoubleB_FluxObsSObserved flux in observed 0.5-2 keV, 1sigma upper limit (FluxObsv_Up1_s)mW.m**-2phot.flux;em.X-ray.softdoubleb2_FluxObsSObserved flux in observed 0.5-2 keV, 2sigma lower limit (FluxObsv_Lo2_s)mW.m**-2stat.errordoubleB2_FluxObsSObserved flux in observed 0.5-2 keV, 2sigma upper limit (FluxObsv_Up2_s)mW.m**-2stat.errordoubleFluxObsBFTObserved flux in observed 2.3-5 keV, best-fit model (FluxObsv_BF_t)mW.m**-2phot.flux;em.X-raydoubleFluxObsMedTObserved flux in observed 2.3-5 keV, posterior median (FluxObsv_Med_t)mW.m**-2phot.flux;em.X-raydoubleb_FluxObsTObserved flux in observed 2.3-5 keV, 1sigma lower limit (FluxObsv_Lo1_t)mW.m**-2phot.flux;em.X-ray.mediumdoubleB_FluxObsTObserved flux in observed 2.3-5 keV, 1sigma upper limit (FluxObsv_Up1_t)mW.m**-2phot.flux;em.X-ray.mediumdoubleb2_FluxObsTObserved flux in observed 2.3-5 keV, 2sigma lower limit (FluxObsv_Lo2_t)mW.m**-2stat.errordoubleB2_FluxObsTObserved flux in observed 2.3-5 keV, 2sigma upper limit (FluxObsv_Up2_t)mW.m**-2stat.errordoubleFluxcBFSAbsorption corrected flux in observed 0.5-2 keV, best-fit model (FluxCorr_BF_s)mW.m**-2phot.flux;em.X-raydoubleFluxcMedSAbsorption corrected flux in observed 0.5-2 keV, posterior median (FluxCorr_Med_s)mW.m**-2phot.flux;em.X-raydoubleb_FluxcSAbsorption corrected flux in observed 0.5-2 keV, 1sigma lower limit (FluxCorr_Lo1_s)mW.m**-2phot.flux;em.X-ray.softdoubleB_FluxcSAbsorption corrected flux in observed 0.5-2 keV, 1sigma upper limit (FluxCorr_Up1_s)mW.m**-2phot.flux;em.X-ray.softdoubleb2_FluxcSAbsorption corrected flux in observed 0.5-2 keV, 2sigma lower limit (FluxCorr_Lo2_s)mW.m**-2stat.errordoubleB2_FluxcSAbsorption corrected flux in observed 0.5-2 keV, 2sigma upper limit (FluxCorr_Up2_s)mW.m**-2stat.errordoubleFluxcBFTAbsorption corrected flux in observed 2.3-5 keV, best-fit model (FluxCorr_BF_t)mW.m**-2phot.flux;em.X-raydoubleFluxcMedTAbsorption corrected flux in observed 2.3-5 keV, posterior median (FluxCorr_Med_t)mW.m**-2phot.flux;em.X-raydoubleb_FluxcTAbsorption corrected flux in observed 2.3-5 keV, 1sigma lower limit (FluxCorr_Lo1_t)mW.m**-2phot.flux;em.X-ray.mediumdoubleB_FluxcTAbsorption corrected flux in observed 2.3-5 keV, 1sigma upper limit (FluxCorr_Up1_t)mW.m**-2phot.flux;em.X-ray.mediumdoubleb2_FluxcTAbsorption corrected flux in observed 2.3-5 keV, 2sigma lower limit (FluxCorr_Lo2_t)mW.m**-2stat.errordoubleB2_FluxcTAbsorption corrected flux in observed 2.3-5 keV, 2sigma upper limit (FluxCorr_Up2_t)mW.m**-2stat.errordoubleFluxIBFSAbsorption corrected flux in rest-frame 0.5-2 keV, best-fit model (FluxIntr_BF_s)mW.m**-2phot.flux;em.X-raydoubleFluxIMedSAbsorption corrected flux in rest-frame 0.5-2 keV, posterior median (FluxIntr_Med_s)mW.m**-2phot.flux;em.X-raydoubleb_FluxISAbsorption corrected flux in rest-frame 0.5-2keV, 1sigma lower limit (FluxIntr_Lo1_s)mW.m**-2phot.flux;em.X-ray.softdoubleb2_FluxISAbsorption corrected flux in rest-frame 0.5-2 keV, 2sigma lower limit (FluxIntr_Lo2_s)mW.m**-2stat.errordoubleB2_FluxISAbsorption corrected flux in rest-frame 0.5-2 keV, 2sigma upper limit (FluxIntr_Up2_s)mW.m**-2stat.errordoubleFluxIBF2keVAbsorption corrected flux at rest-frame 2keV, best- fit (FluxIntr_BF_2keV)mW.m**-2.eV**-1phot.flux;em.X-raydoubleFluxIMed2keVAbsorption corrected flux at rest-frame 2keV, median (FluxIntr_Med_2keV)mW.m**-2.eV**-1phot.flux;em.X-raydoubleb_FluxI2keVAbsorption corrected flux at rest-frame 2keV, 1sigma lower limit (FluxIntr_Lo1_2keV)mW.m**-2.eV**-1phot.fluxdoubleB_FluxI2keVAbsorption corrected flux at rest-frame 2keV, 1sigma upper limit (FluxIntr_Up1_2keV)mW.m**-2.eV**-1phot.fluxdoubleb2_FluxI2keVAbsorption corrected flux at rest-frame 2keV, 2sigma lower limit (FluxIntr_Lo2_2keV)mW.m**-2.eV**-1stat.errordoubleB2_FluxI2keVAbsorption corrected flux at rest-frame 2keV, 2sigma upper limit (FluxIntr_Up2_2keV)mW.m**-2.eV**-1stat.errordoubleLumIBFS? Intrinsic luminosity in rest-frame 0.5-2 keV, best-fit model (LumiIntr_BF_s)1e-07Wphys.luminosity;em.X-raydoublenullableLumIMedS? Intrinsic luminosity in rest-frame 0.5-2 keV, posterior median (LumiIntr_Med_s)1e-07Wphys.luminosity;em.X-raydoublenullableb_LumIS? Intrinsic luminosity in rest-frame 0.5-2 keV, 1sigma lower limit (LumiIntr_Lo1_s)1e-07Wphys.luminosity;em.X-ray.softdoublenullableB_LumIS? Intrinsic luminosity in rest-frame 0.5-2 keV, 1sigma upper limit (LumiIntr_Up1_s)1e-07Wphys.luminosity;em.X-ray.softdoublenullableb2_LumIS? Intrinsic luminosity in rest-frame 0.5-2 keV, 2sigma lower limit (LumiIntr_Lo2_s)1e-07Wstat.errordoublenullableB2_LumIS? Intrinsic luminosity in rest-frame 0.5-2 keV, 2sigma upper limit (LumiIntr_Up2_s)1e-07Wstat.errordoublenullableLumIBF2keV? Intrinsic luminosity at rest-frame 2keV, best-fit model (LumiIntr_BF_2keV)1e-07W.eV**-1phys.luminosity;em.X-raydoublenullableLumIMed2keV? Intrinsic luminosity at rest-frame 2keV, posterior median (LumiIntr_Med_2keV)1e-07W.eV**-1phys.luminosity;em.X-raydoublenullableb_LumI2keV? Intrinsic luminosity at rest-frame 2keV, 1sigma lower limit (LumiIntr_Lo1_2keV)1e-07W.eV**-1phys.luminositydoublenullableB_LumI2keV? Intrinsic luminosity at rest-frame 2keV, 1sigma upper limit (LumiIntr_Up1_2keV)1e-07W.eV**-1phys.luminositydoublenullableb2_LumI2keV? Intrinsic luminosity at rest-frame 2keV, 2sigma lower limit (LumiIntr_Lo2_2keV)1e-07W.eV**-1stat.errordoublenullableB2_LumI2keV? Intrinsic luminosity at rest-frame 2keV, 2sigma upper limit (LumiIntr_Up2_2keV)1e-07W.eV**-1stat.errordoublenullableGammaMedpower-law slope, posterior median (Gamma_Med)spect.indexdoubleb_Gammapower-law slope, percentile lower limit (Gamma_Lo)arith.grad;stat.mindoubleB_Gammapower-law slope, percentile upper limit (Gamma_Up)arith.grad;stat.maxdoubleGammaMeanpower-law slope, mean (Gamma_Mean)spect.indexdoubles_Gammapower-law slope, standard deviation (Gamma_Std)stat.stdevdoublelognHMedlog AGN column density, posterior median (lognH_Med)log(cm**-2)phys.columnDensity;stat.mediandoubleb_lognHlog AGN column density, percentile lower limit (lognH_Lo)log(cm**-2)phys.columnDensity;stat.mindoubleB_lognHlog AGN column density, percentile upper limit (lognH_Up)log(cm**-2)phys.columnDensity;stat.maxdoublelognHMeanlog AGN column density, mean (lognH_Mean)log(cm**-2)phys.columnDensity;stat.meandoubleb_logPowNlog power-law normalization, percentile lower limit (logPowNorm_Lo)ph.keV**-1.cm**-2.s**-1arith.zp;arith.ratiodoubleB_logPowNlog power-law normalization, percentile upper limit (logPowNorm_Up)ph.keV**-1.cm**-2.s**-1arith.zp;arith.ratiodoublelogPowNMeanlog power-law normalization, mean (logPowNorm_Mean)ph.keV**-1.cm**-2.s**-1stat.fit.paramdoubles_logPowNlog power-law normalization, standard deviation (logPowNorm_Std)ph.keV**-1.cm**-2.s**-1arith.zp;arith.ratiodoublelogBkgNMedlog background normalization, posterior median (logBkgNorm_Med)instr.backgrounddoubleb_logBkgNlog background normalization, percentile lower limit (logBkgNorm_Lo)instr.background;arith.ratiodoubleB_logBkgNlog background normalization, percentile upper limit (logBkgNorm_Up)instr.background;arith.ratiodoublelogBkgNMeanlog background normalization, mean (logBkgNorm_Mean)instr.backgrounddoubles_logBkgNlog background normalization, standard deviation (logBkgNorm_Std)instr.background;arith.ratiodoublechi25? Chi^2 of the best-fit model against the rebinned data (>=25 cts/bin) (chi25)stat.fit.chi2doublenullabledof25? DOF of the rebinned data, which has at least 25 counts per bin (dof25)stat.fit.dofintnullablelogZlog10 Bayesian evidence (logZ)stat.fit.paramdoubleNHclass[1/4] Class of AGN NH measurement with model 1 (single-powerlaw) (NHclass) (1)src.classintPaperIDisplay the Paper I (Brunner et al., Cat. J/A+A/661/A1) datameta.ref.urlcharPaperIIDisplay the Paper II (Salvato et al., Cat. J/A+A/661/A3) datameta.ref.urlcharJ/A+A/661/A5/table5Double-powerlaw resultslogFracKL? Constant factor multiplied to the soft power-law, KL divergence (in nats units) (logFrac_KL)stat.fit.paramdoublenullablePaperIDisplay the Paper I (Brunner et al., Cat. J/A+A/661/A1) datameta.ref.urlcharPaperIIDisplay the Paper II (Salvato et al., Cat. J/A+A/661/A3) datameta.ref.urlcharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintID-SRC[1/32683] ID of the sources in the eFEDS main X-ray catalog (Paper I) (ID_SRC)meta.id;meta.mainintz[-0.01/8.0] The redshift adopted for the spectral model (Redshift)src.redshiftdoubledGmKLSoft-powerlaw slope minus primary-powerlaw slope, KL divergence (in nats units) (dGm_KL)stat.fit.paramdoubleb_dGmHSoft-powerlaw slope minus primary-powerlaw slope, HDI lower limit (dGm_HLo)arith.grad;stat.fit.omcdoubleB_dGmHSoft-powerlaw slope minus primary-powerlaw slope, HDI upper limit (dGm_HUp)arith.grad;stat.fit.omcdoubleGammaKL? power-law slope, KL divergence (in nats units) (Gamma_KL)stat.fit.paramdoublenullableb_GammaHpower-law slope, HDI lower limit (Gamma_HLo)arith.grad;stat.mindoubleB_GammaHpower-law slope, HDI upper limit (Gamma_HUp)arith.grad;stat.maxdoublelognHKLlog AGN column density, KL divergence (in nats units) (lognH_KL)stat.fit.paramdoubleb_lognHHlog AGN column density, HDI lower limit (lognH_HLo)log(cm**-2)phys.columnDensity;stat.mindoubleB_lognHHlog AGN column density, HDI upper limit (lognH_HUp)log(cm**-2)phys.columnDensity;stat.maxdoublelogPowNKLlog power-law normalization, KL divergence (in nats units) (logPowNorm_KL)stat.fit.paramdoubleb_logPowNHlog power-law normalization, HDI lower limit (logPowNorm_HLo)log(ph.keV**-1.cm**-2.s**-1)arith.zp;arith.ratiodoubleB_logPowNHlog power-law normalization, HDI upper limit (logPowNorm_HUp)log(ph.keV**-1.cm**-2.s**-1)arith.zp;arith.ratiodoubleb_logFracHConstant factor multiplied to the soft power-law, HDI lower limit (logFrac_HLo)arith.factor;arith.zpdoubleB_logFracHConstant factor multiplied to the soft power-law, HDI upper limit (logFrac_HUp)arith.factor;arith.zpdoubledGmBFSoft-powerlaw slope minus primary-powerlaw slope, best-fit model (dGm_BF)stat.fit.paramdoubleGammaBFpower-law slope, best-fit model (Gamma_BF)spect.indexdoublelognHBFlog AGN column density, best-fit model (lognH_BF)log(cm**-2)phys.columnDensity;meta.modelleddoublelogPowNBFlog power-law normalization, best-fit model (logPowNorm_BF)log(ph.keV**-1.cm**-2.s**-1)stat.fit.paramdoublelogFracBFConstant factor multiplied to the soft power-law, best-fit model (logFrac_BF)stat.fit.paramdoubleFluxObsBFSObserved flux in observed 0.5-2 keV, best-fit model (FluxObsv_BF_s)mW.m**-2phot.flux;em.X-raydoubleFluxObsMedSObserved flux in observed 0.5-2 keV, posterior median (FluxObsv_Med_s)mW.m**-2phot.flux;em.X-raydoubleb_FluxObsSObserved flux in observed 0.5-2 keV, 1sigma lower limit (FluxObsv_Lo1_s)mW.m**-2phot.flux;em.X-ray.softdoubleB_FluxObsSObserved flux in observed 0.5-2 keV, 1sigma upper limit (FluxObsv_Up1_s)mW.m**-2phot.flux;em.X-ray.softdoubleb2_FluxObsSObserved flux in observed 0.5-2 keV, 2sigma lower limit (FluxObsv_Lo2_s)mW.m**-2stat.errordoubleB2_FluxObsSObserved flux in observed 0.5-2 keV, 2sigma upper limit (FluxObsv_Up2_s)mW.m**-2stat.errordoubleFluxObsBFTObserved flux in observed 2.3-5 keV, best-fit model (FluxObsv_BF_t)mW.m**-2phot.flux;em.X-raydoubleFluxObsMedTObserved flux in observed 2.3-5 keV, posterior median (FluxObsv_Med_t)mW.m**-2phot.flux;em.X-raydoubleb_FluxObsTObserved flux in observed 2.3-5 keV, 1sigma lower limit (FluxObsv_Lo1_t)mW.m**-2phot.flux;em.X-ray.mediumdoubleB_FluxObsTObserved flux in observed 2.3-5 keV, 1sigma upper limit (FluxObsv_Up1_t)mW.m**-2phot.flux;em.X-ray.mediumdoubleb2_FluxObsTObserved flux in observed 2.3-5 keV, 2sigma lower limit (FluxObsv_Lo2_t)mW.m**-2stat.errordoubleB2_FluxObsTObserved flux in observed 2.3-5 keV, 2sigma upper limit (FluxObsv_Up2_t)mW.m**-2stat.errordoubleFluxCBFSAbsorption corrected flux in observed 0.5-2 keV, best-fit model (FluxCorr_BF_s)mW.m**-2phot.flux;em.X-raydoubleFluxCMedSAbsorption corrected flux in observed 0.5-2 keV, posterior median (FluxCorr_Med_s)mW.m**-2phot.flux;em.X-raydoubleb_FluxCSAbsorption corrected flux in observed 0.5-2 keV, 1sigma lower limit (FluxCorr_Lo1_s)mW.m**-2phot.flux;em.X-ray.softdoubleB_FluxCSAbsorption corrected flux in observed 0.5-2 keV, 1sigma upper limit (FluxCorr_Up1_s)mW.m**-2phot.flux;em.X-ray.softdoubleb2_FluxCSAbsorption corrected flux in observed 0.5-2 keV, 2sigma lower limit (FluxCorr_Lo2_s)mW.m**-2stat.errordoubleB2_FluxCSAbsorption corrected flux in observed 0.5-2 keV, 2sigma upper limit (FluxCorr_Up2_s)mW.m**-2stat.errordoubleFluxCBFTAbsorption corrected flux in observed 2.3-5 keV, best-fit model (FluxCorr_BF_t)mW.m**-2phot.flux;em.X-raydoubleFluxCMedTAbsorption corrected flux in observed 2.3-5 keV, posterior median (FluxCorr_Med_t)mW.m**-2phot.flux;em.X-raydoubleb_FluxCTAbsorption corrected flux in observed 2.3-5 keV, 1sigma lower limit (FluxCorr_Lo1_t)mW.m**-2phot.flux;em.X-ray.mediumdoubleB_FluxCTAbsorption corrected flux in observed 2.3-5 keV, 1sigma upper limit (FluxCorr_Up1_t)mW.m**-2phot.flux;em.X-ray.mediumdoubleb2_FluxCTAbsorption corrected flux in observed 2.3-5 keV, 2sigma lower limit (FluxCorr_Lo2_t)mW.m**-2stat.errordoubleB2_FluxCTAbsorption corrected flux in observed 2.3-5 keV, 2sigma upper limit (FluxCorr_Up2_t)mW.m**-2stat.errordoubleFluxIBFSAbsorption corrected flux in rest-frame 0.5-2 keV, best-fit model (FluxIntr_BF_s)mW.m**-2phot.flux;em.X-raydoubleFluxIMedSAbsorption corrected flux in rest-frame 0.5-2 keV, posterior median (FluxIntr_Med_s)mW.m**-2phot.flux;em.X-raydoubleb_FluxISAbsorption corrected flux in rest-frame 0.5-2keV, 1sigma lower limit (FluxIntr_Lo1_s)mW.m**-2phot.flux;em.X-ray.softdoubleB_FluxISAbsorption corrected flux in rest-frame 0.5-2keV, 1sigma upper limit (FluxIntr_Up1_s)mW.m**-2phot.flux;em.X-ray.softdoubleb2_FluxISAbsorption corrected flux in rest-frame 0.5-2 keV, 2sigma lower limit (FluxIntr_Lo2_s)mW.m**-2stat.errordoubleB2_FluxISAbsorption corrected flux in rest-frame 0.5-2 keV, 2sigma upper limit (FluxIntr_Up2_s)mW.m**-2stat.errordoubleFluxIBF2keVAbsorption corrected flux at rest-frame 2keV, best-fit (FluxIntr_BF_2keV)mW.m**-2.eV**-1phot.flux;em.X-raydoubleFluxIMed2keVAbsorption corrected flux at rest-frame 2keV, median (FluxIntr_Med_2keV)mW.m**-2.eV**-1phot.flux;em.X-raydoubleb_FluxI2keVAbsorption corrected flux at rest-frame 2keV, 1sigma lower limit (FluxIntr_Lo1_2keV)mW.m**-2.eV**-1phot.fluxdoubleB_FluxI2keVAbsorption corrected flux at rest-frame 2keV, 1sigma upper limit (FluxIntr_Up1_2keV)mW.m**-2.eV**-1phot.fluxdoubleb2_FluxI2keVAbsorption corrected flux at rest-frame 2keV, 2sigma lower limit (FluxIntr_Lo2_2keV)mW.m**-2.eV**-1stat.errordoubleB2_FluxI2keVAbsorption corrected flux at rest-frame 2keV, 2sigma upper limit (FluxIntr_Up2_2keV)mW.m**-2.eV**-1stat.errordoubleLumIBFS? Intrinsic luminosity in rest-frame 0.5-2 keV, best-fit model (LumiIntr_BF_s)1e-07Wphys.luminosity;em.X-raydoublenullableLumIMedS? Intrinsic luminosity in rest-frame 0.5-2 keV, posterior median (LumiIntr_Med_s)1e-07Wphys.luminosity;em.X-raydoublenullableb_LumIS? Intrinsic luminosity in rest-frame 0.5-2 keV, 1sigma lower limit (LumiIntr_Lo1_s)1e-07Wphys.luminosity;em.X-ray.softdoublenullableB_LumIS? Intrinsic luminosity in rest-frame 0.5-2 keV, 1sigma upper limit (LumiIntr_Up1_s)1e-07Wphys.luminosity;em.X-ray.softdoublenullableb2_LumIS? Intrinsic luminosity in rest-frame 0.5-2 keV, 2sigma lower limit (LumiIntr_Lo2_s)1e-07Wstat.errordoublenullableB2_LumIS? Intrinsic luminosity in rest-frame 0.5-2 keV, 2sigma upper limit (LumiIntr_Up2_s)1e-07Wstat.errordoublenullableLumIBF2keV? Intrinsic luminosity at rest-frame 2keV, best-fit model (LumiIntr_BF_2keV)1e-07W.eV**-1phys.luminosity;em.X-raydoublenullableLumIMed2keV? Intrinsic luminosity at rest-frame 2keV, posterior median (LumiIntr_Med_2keV)1e-07W.eV**-1phys.luminosity;em.X-raydoublenullableb_LumI2keV? Intrinsic luminosity at rest-frame 2keV, 1sigma lower limit (LumiIntr_Lo1_2keV)1e-07W.eV**-1phys.luminositydoublenullableB_LumI2keV? Intrinsic luminosity at rest-frame 2keV, 1sigma upper limit (LumiIntr_Up1_2keV)1e-07W.eV**-1phys.luminositydoublenullableb2_LumI2keV? Intrinsic luminosity at rest-frame 2keV, 2sigma lower limit (LumiIntr_Lo2_2keV)1e-07W.eV**-1stat.errordoublenullableB2_LumI2keV? Intrinsic luminosity at rest-frame 2keV, 2sigma upper limit (LumiIntr_Up2_2keV)1e-07W.eV**-1stat.errordoublenullabledGmMedSoft-powerlaw slope minus primary-powerlaw slope, posterior median (dGm_Med)stat.fit.paramdoubleb_dGmSoft-powerlaw slope minus primary-powerlaw slope, 1sigma lower limit (dGm_Lo)arith.grad;stat.fit.omcdoubleB_dGmSoft-powerlaw slope minus primary-powerlaw slope, 1sigma upper limit (dGm_Up)arith.grad;stat.fit.omcdoubledGmMeanSoft-powerlaw slope minus primary-powerlaw slope, mean (dGm_Mean)stat.fit.paramdoubles_dGmSoft-powerlaw slope minus primary-powerlaw slope, standard deviation (dGm_Std)arith.grad;stat.fit.omcdoubleGammaMedpower-law slope, posterior median (Gamma_Med)spect.indexdoubleb_Gammapower-law slope, percentile lower limit (Gamma_Lo)arith.grad;stat.mindoubleB_Gammapower-law slope, percentile upper limit (Gamma_Up)arith.grad;stat.maxdoubleGammaMeanpower-law slope, mean (Gamma_Mean)spect.indexdoubles_Gammapower-law slope, standard deviation (Gamma_Std)stat.stdevdoublelognHMedlog AGN column density, posterior median (lognH_Med)log(cm**-2)phys.columnDensity;stat.mediandoubleb_lognHlog AGN column density, percentile lower limit (lognH_Lo)log(cm**-2)phys.columnDensity;stat.mindoubleB_lognHlog AGN column density, percentile upper limit (lognH_Up)log(cm**-2)phys.columnDensity;stat.maxdoublelognHMeanlog AGN column density, mean (lognH_Mean)log(cm**-2)phys.columnDensity;stat.meandoubles_lognHlog AGN column density, standard deviation (lognH_Std)log(cm**-2)stat.stdev;phys.columnDensitydoublelogPowNMedlog power-law normalization, posterior median (logPowNorm_Med)log(ph.keV**-1.cm**-2.s**-1)stat.fit.paramdoubleb_logPowNlog power-law normalization, percentile lower limit (logPowNorm_Lo)log(ph.keV**-1.cm**-2.s**-1)arith.zp;arith.ratiodoubleB_logPowNlog power-law normalization, percentile upper limit (logPowNorm_Up)log(ph.keV**-1.cm**-2.s**-1)arith.zp;arith.ratiodoublelogPowNMeanlog power-law normalization, mean (logPowNorm_Mean)log(ph.keV**-1.cm**-2.s**-1)stat.fit.paramdoubles_logPowNlog power-law normalization, standard deviation (logPowNorm_Std)log(ph.keV**-1.cm**-2.s**-1)arith.zp;arith.ratiodoublelogFracMedConstant factor multiplied to the soft power-law, posterior median (logFrac_Med)stat.fit.paramdoubleb_logFracConstant factor multiplied to the soft power-law, 1sigma lower limit (logFrac_Lo)arith.factor;arith.zpdoubleB_logFracConstant factor multiplied to the soft power-law, 1sigma upper limit (logFrac_Up)arith.factor;arith.zpdoublelogFracMeanConstant factor multiplied to the soft power-law, mean (logFrac_Mean)stat.fit.paramdoubles_logFracConstant factor multiplied to the soft power-law, standard deviation (logFrac_Std)arith.factor;arith.zpdoublelogBkgNMedlog background normalization, posterior median (logBkgNorm_Med)instr.backgrounddoubleb_logBkgNlog background normalization, percentile lower limit (logBkgNorm_Lo)instr.background;arith.ratiodoubleB_logBkgNlog background normalization, percentile upper limit (logBkgNorm_Up)instr.background;arith.ratiodoublelogBkgNMeanlog background normalization, mean (logBkgNorm_Mean)instr.backgrounddoubles_logBkgNlog background normalization, standard deviation (logBkgNorm_Std)instr.background;arith.ratiodoublechi25? Chi^2 of the best-fit model against the rebinned data (>=25 cts/bin) (chi25)stat.fit.chi2doublenullabledof25? DOF of the rebinned data, which has at least 25 counts per bin (dof25)stat.fit.dofintnullablelogZlog10 Bayesian evidence (logZ)stat.fit.paramdoubleJ/A+A/661/A5/table6Powerlaw+blackbody resultsb_GammaHpower-law slope, HDI lower limit (Gamma_HLo)arith.grad;stat.mindoubles_lognHlog AGN column density, standard deviation (lognH_Std)log(cm**-2)stat.stdev;phys.columnDensitydoublelogPowNMedlog power-law normalization, posterior median (logPowNorm_Med)log(ph.keV**-1.cm**-2.s**-1)stat.fit.paramdoublerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintID-SRC[1/32683] ID of the sources in the eFEDS main X-ray catalog (Paper I) (ID_SRC)meta.id;meta.mainintz[-0.01/8.0] The redshift adopted for the spectral model (Redshift)src.redshiftdoubleGammaKLpower-law slope, KL divergence (in nats units) (Gamma_KL)stat.fit.paramdoubleB_GammaHpower-law slope, HDI upper limit (Gamma_HUp)arith.grad;stat.maxdoublelognHKLlog AGN column density, KL divergence (in nats units) (lognH_KL)stat.fit.paramdoubleb_lognHHlog AGN column density, HDI lower limit (lognH_HLo)log(cm**-2)phys.columnDensity;stat.mindoubleB_lognHHlog AGN column density, HDI upper limit (lognH_HUp)log(cm**-2)phys.columnDensity;stat.maxdoublelogPowNKLlog power-law normalization, KL divergence (in nats units) (logPowNorm_KL)stat.fit.paramdoubleb_logPowNHlog power-law normalization, HDI lower limit (logPowNorm_HLo)log(ph.keV**-1.cm**-2.s**-1)arith.zp;arith.ratiodoubleB_logPowNHlog power-law normalization, HDI upper limit (logPowNorm_HUp)log(ph.keV**-1.cm**-2.s**-1)arith.zp;arith.ratiodoublelogkTKLlog temperature, KL divergence (in nats units) (logkT_KL)stat.fit.paramdoubleb_logkTHlog temperature, HDI lower limit (logkT_HLo)log(keV)phys.temperature;stat.mindoubleB_logkTHlog temperature, HDI upper limit (logkT_HUp)log(keV)phys.temperature;stat.maxdoublelogBBNKLlog blackbody normalization, KL divergence (in nats units) (logBBNorm_KL)stat.fit.paramdoubleb_logBBNHlog blackbody normalization in 10^+31^erg/pc^2^, HDI lower limit (logBBNorm_HLo)log(1e+24W.pc**-2)arith.zp;arith.ratiodoubleB_logBBNHlog blackbody normalization in 10^+31^erg/pc^2^, HDI upper limit (logBBNorm_HUp)log(1e+24W.pc**-2)arith.zp;arith.ratiodoubleGammaBFpower-law slope, best-fit model (Gamma_BF)spect.indexdoublelognHBFlog AGN column density, best-fit model (lognH_BF)log(cm**-2)phys.columnDensitydoublelogPowNBFlog power- law normalization, best-fit model (logPowNorm_BF)log(ph.keV**-1.cm**-2.s**-1)stat.fit.paramdoublelogkTBFlog temperature, best- fit model (logkT_BF)log(keV)phys.temperaturedoublelogBBNBFlog blackbody normalization in 10^+31^erg/pc^2^, best-fit model (logBBNorm_BF)log(1e+24W.pc**-2)stat.fit.paramdoubleFluxObsBFSObserved flux in observed 0.5-2 keV, best-fit model (FluxObsv_BF_s)mW.m**-2phot.flux;em.X-raydoubleFluxObsMedSObserved flux in observed 0.5-2 keV, posterior median (FluxObsv_Med_s)mW.m**-2phot.flux;em.X-raydoubleb_FluxObsSObserved flux in observed 0.5-2 keV, 1sigma lower limit (FluxObsv_Lo1_s)mW.m**-2phot.flux;em.X-ray.softdoubleB_FluxObsSObserved flux in observed 0.5-2 keV, 1sigma upper limit (FluxObsv_Up1_s)mW.m**-2phot.flux;em.X-ray.softdoubleb2_FluxObsSObserved flux in observed 0.5-2 keV, 2sigma lower limit (FluxObsv_Lo2_s)mW.m**-2stat.errordoubleB2_FluxObsSObserved flux in observed 0.5-2 keV, 2sigma upper limit (FluxObsv_Up2_s)mW.m**-2stat.errordoubleFluxObsBFTObserved flux in observed 2.3-5 keV, best-fit model (FluxObsv_BF_t)mW.m**-2phot.flux;em.X-raydoubleFluxObsMedTObserved flux in observed 2.3-5 keV, posterior median (FluxObsv_Med_t)mW.m**-2phot.flux;em.X-raydoubleb_FluxObsTObserved flux in observed 2.3-5 keV, 1sigma lower limit (FluxObsv_Lo1_t)mW.m**-2phot.flux;em.X-ray.mediumdoubleB_FluxObsTObserved flux in observed 2.3-5 keV, 1sigma upper limit (FluxObsv_Up1_t)mW.m**-2phot.flux;em.X-ray.mediumdoubleb2_FluxObsTObserved flux in observed 2.3-5 keV, 2sigma lower limit (FluxObsv_Lo2_t)mW.m**-2stat.errordoubleB2_FluxObsTObserved flux in observed 2.3-5 keV, 2sigma upper limit (FluxObsv_Up2_t)mW.m**-2stat.errordoubleFluxCBFSAbsorption corrected flux in observed 0.5-2 keV, best-fit model (FluxCorr_BF_s)mW.m**-2phot.flux;em.X-raydoubleFluxCMedSAbsorption corrected flux in observed 0.5-2 keV, posterior median (FluxCorr_Med_s)mW.m**-2phot.flux;em.X-raydoubleb_FluxCSAbsorption corrected flux in observed 0.5-2 keV, 1sigma lower limit (FluxCorr_Lo1_s)mW.m**-2phot.flux;em.X-ray.softdoubleB_FluxCSAbsorption corrected flux in observed 0.5-2 keV, 1sigma upper limit (FluxCorr_Up1_s)mW.m**-2phot.flux;em.X-ray.softdoubleb2_FluxCSAbsorption corrected flux in observed 0.5-2 keV, 2sigma lower limit (FluxCorr_Lo2_s)mW.m**-2stat.errordoubleB2_FluxCSAbsorption corrected flux in observed 0.5-2 keV, 2sigma upper limit (FluxCorr_Up2_s)mW.m**-2stat.errordoubleFluxCBFTAbsorption corrected flux in observed 2.3-5 keV, best-fit model (FluxCorr_BF_t)mW.m**-2phot.flux;em.X-raydoubleFluxCMedTAbsorption corrected flux in observed 2.3-5 keV, posterior median (FluxCorr_Med_t)mW.m**-2phot.flux;em.X-raydoubleb_FluxCTAbsorption corrected flux in observed 2.3-5 keV, 1sigma lower limit (FluxCorr_Lo1_t)mW.m**-2phot.flux;em.X-ray.mediumdoubleB_FluxCTAbsorption corrected flux in observed 2.3-5 keV, 1sigma upper limit (FluxCorr_Up1_t)mW.m**-2phot.flux;em.X-ray.mediumdoubleb2_FluxCTAbsorption corrected flux in observed 2.3-5 keV, 2sigma lower limit (FluxCorr_Lo2_t)mW.m**-2stat.errordoubleB2_FluxCTAbsorption corrected flux in observed 2.3-5 keV, 2sigma upper limit (FluxCorr_Up2_t)mW.m**-2stat.errordoubleFluxIBFSAbsorption corrected flux in rest-frame 0.5-2 keV, best-fit model (FluxIntr_BF_s)mW.m**-2phot.flux;em.X-raydoubleFluxIMedSAbsorption corrected flux in rest-frame 0.5-2 keV, posterior median (FluxIntr_Med_s)mW.m**-2phot.flux;em.X-raydoubleb_FluxISAbsorption corrected flux in rest-frame 0.5-2keV, 1sigma lower limit (FluxIntr_Lo1_s)mW.m**-2phot.flux;em.X-ray.softdoubleB_FluxISAbsorption corrected flux in rest-frame 0.5-2keV, 1sigma upper limit (FluxIntr_Up1_s)mW.m**-2phot.flux;em.X-ray.softdoubleb2_FluxISAbsorption corrected flux in rest-frame 0.5-2 keV, 2sigma lower limit (FluxIntr_Lo2_s)mW.m**-2stat.errordoubleB2_FluxISAbsorption corrected flux in rest-frame 0.5-2 keV, 2sigma upper limit (FluxIntr_Up2_s)mW.m**-2stat.errordoubleFluxIBF2keVAbsorption corrected flux at rest-frame 2keV, best-fit (FluxIntr_BF_2keV)mW.m**-2.eV**-1phot.flux;em.X-raydoubleFluxIMed2keVAbsorption corrected flux at rest-frame 2keV, median (FluxIntr_Med_2keV)mW.m**-2.eV**-1phot.flux;em.X-raydoubleb_FluxI2keVAbsorption corrected flux at rest-frame 2keV, 1sigma lower limit (FluxIntr_Lo1_2keV)mW.m**-2.eV**-1phot.fluxdoubleB_FluxI2keVAbsorption corrected flux at rest-frame 2keV, 1sigma upper limit (FluxIntr_Up1_2keV)mW.m**-2.eV**-1phot.fluxdoubleb2_FluxI2keVAbsorption corrected flux at rest-frame 2keV, 2sigma lower limit (FluxIntr_Lo2_2keV)mW.m**-2.eV**-1stat.errordoubleB2_FluxI2keVAbsorption corrected flux at rest-frame 2keV, 2sigma upper limit (FluxIntr_Up2_2keV)mW.m**-2.eV**-1stat.errordoubleLumIBFS? Intrinsic luminosity in rest-frame 0.5-2 keV, best-fit model (LumiIntr_BF_s)1e-07Wphys.luminosity;em.X-raydoublenullableLumIMedS? Intrinsic luminosity in rest-frame 0.5-2 keV, posterior median (LumiIntr_Med_s)1e-07Wphys.luminosity;em.X-raydoublenullableb_LumIS? Intrinsic luminosity in rest-frame 0.5-2 keV, 1sigma lower limit (LumiIntr_Lo1_s)1e-07Wphys.luminosity;em.X-ray.softdoublenullableB_LumIS? Intrinsic luminosity in rest-frame 0.5-2 keV, 1sigma upper limit (LumiIntr_Up1_s)1e-07Wphys.luminosity;em.X-ray.softdoublenullableb2_LumIS? Intrinsic luminosity in rest-frame 0.5-2 keV, 2sigma lower limit (LumiIntr_Lo2_s)1e-07Wstat.errordoublenullableB2_LumIS? Intrinsic luminosity in rest-frame 0.5-2 keV, 2sigma upper limit (LumiIntr_Up2_s)1e-07Wstat.errordoublenullableLumIBF2keV? Intrinsic luminosity at rest-frame 2keV, best-fit model (LumiIntr_BF_2keV)1e-07W.eV**-1phys.luminosity;em.X-raydoublenullableLumIMed2keV? Intrinsic luminosity at rest-frame 2keV, posterior median (LumiIntr_Med_2keV)1e-07W.eV**-1phys.luminosity;em.X-raydoublenullableb_LumI2keV? Intrinsic luminosity at rest-frame 2keV, 1sigma lower limit (LumiIntr_Lo1_2keV)1e-07W.eV**-1phys.luminositydoublenullableB_LumI2keV? Intrinsic luminosity at rest-frame 2keV, 1sigma upper limit (LumiIntr_Up1_2keV)1e-07W.eV**-1phys.luminositydoublenullableb2_LumI2keV? Intrinsic luminosity at rest-frame 2keV, 2sigma lower limit (LumiIntr_Lo2_2keV)1e-07W.eV**-1stat.errordoublenullableB2_LumI2keV? Intrinsic luminosity at rest-frame 2keV, 2sigma upper limit (LumiIntr_Up2_2keV)1e-07W.eV**-1stat.errordoublenullableGammaMedpower-law slope, posterior median (Gamma_Med)spect.indexdoubleb_Gammapower-law slope, percentile lower limit (Gamma_Lo)arith.grad;stat.mindoubleB_Gammapower-law slope, percentile upper limit (Gamma_Up)arith.grad;stat.maxdoubleGammaMeanpower-law slope, mean (Gamma_Mean)spect.indexdoubles_Gammapower-law slope, standard deviation (Gamma_Std)stat.stdevdoublelognHMedlog AGN column density, posterior median (lognH_Med)log(cm**-2)phys.columnDensitydoubleb_lognHlog AGN column density, percentile lower limit (lognH_Lo)log(cm**-2)phys.columnDensity;stat.mindoubleB_lognHlog AGN column density, percentile upper limit (lognH_Up)log(cm**-2)phys.columnDensity;stat.maxdoublelognHMeanlog AGN column density, mean (lognH_Mean)log(cm**-2)phys.columnDensitydoubleb_logPowNlog power-law normalization, percentile lower limit (logPowNorm_Lo)log(ph.keV**-1.cm**-2.s**-1)arith.zp;arith.ratiodoubleB_logPowNlog power-law normalization, percentile upper limit (logPowNorm_Up)log(ph.keV**-1.cm**-2.s**-1)arith.zp;arith.ratiodoublelogPowNMeanlog power-law normalization, mean (logPowNorm_Mean)log(ph.keV**-1.cm**-2.s**-1)stat.fit.paramdoubles_logPowNlog power-law normalization, standard deviation (logPowNorm_Std)log(ph.keV**-1.cm**-2.s**-1)arith.zp;arith.ratiodoublelogkTMedlog temperature, posterior median (logkT_Med)log(keV)phys.temperaturedoubleb_logkTlog temperature, percentile lower limit (logkT_Lo)log(keV)phys.temperature;stat.mindoubleB_logkTlog temperature, percentile upper limit (logkT_Up)log(keV)phys.temperature;stat.maxdoublelogkTMeanlog temperature, mean (logkT_Mean)log(keV)phys.temperaturedoubles_logkTlog temperature, standard deviation (logkT_Std)log(keV)stat.stdev;phys.temperaturedoublelogBBNMedlog blackbody normalization in 10^+31^erg/s/pc^2^, posterior median (logBBNorm_Med)log(1e+24W.pc**-2)stat.fit.paramdoubleb_logBBNlog blackbody normalization in 10^+31^erg/s/pc^2^, percentile lower limit (logBBNorm_Lo)log(1e+24W.pc**-2)arith.zp;arith.ratiodoubleB_logBBNlog blackbody normalization in 10^+31^erg/s/pc^2^, percentile upper limit (logBBNorm_Up)log(1e+24W.pc**-2)arith.zp;arith.ratiodoublelogBBNMeanlog blackbody normalization in 10^+31^erg/s/pc^2^, mean (logBBNorm_Mean)log(1e+24W.pc**-2)stat.fit.paramdoubles_logBBNlog blackbody normalization in 10^+31^erg/s/pc^2^, standard deviation (logBBNorm_Std)log(1e+24W.pc**-2)arith.zp;arith.ratiodoublelogBkgNMedlog background normalization, posterior median (logBkgNorm_Med)instr.backgrounddoubleb_logBkgNlog background normalization, percentile lower limit (logBkgNorm_Lo)instr.background;arith.ratiodoubleB_logBkgNlog background normalization, percentile upper limit (logBkgNorm_Up)instr.background;arith.ratiodoublelogBkgNMeanlog background normalization, mean (logBkgNorm_Mean)instr.backgrounddoubles_logBkgNlog background normalization, standard deviation (logBkgNorm_Std)instr.background;arith.ratiodoublechi25? Chi^2 of the best-fit model against the rebinned data (>=25 cts/bin) (chi25)stat.fit.chi2doublenullabledof25? DOF of the rebinned data, which has at least 25 counts per bin (dof25)stat.fit.dofintnullablelogZlog10 Bayesian evidence (logZ)stat.fit.paramdoublelogRbblog blackbody relative strength at 1keV (logRbb)stat.fit.paramdoublePaperIDisplay the Paper I (Brunner et al., Cat. J/A+A/661/A1) datameta.ref.urlcharPaperIIDisplay the Paper II (Salvato et al., Cat. J/A+A/661/A3) datameta.ref.urlcharJ/A+A/661/A5/table7Gamma-fixed-powerlaw resultsb_lognHHlog AGN column density, HDI lower limit (lognH_HLo)log(cm**-2)phys.columnDensity;stat.mindoubleb_LumI2keV? Intrinsic luminosity at rest-frame 2keV, 1sigma lower limit (LumiIntr_Lo1_2keV)1e-07W.eV**-1phys.luminositydoublenullableB_LumI2keV? Intrinsic luminosity at rest-frame 2keV, 1sigma upper limit (LumiIntr_Up1_2keV)1e-07W.eV**-1phys.luminositydoublenullablelognHMedlog AGN column density, posterior median (lognH_Med)log(cm**-2)phys.columnDensitydoublerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintID-SRC[1/32683] ID of the sources in the eFEDS main X-ray catalog (Paper I) (ID_SRC)meta.id;meta.mainintz[-0.01/8.0] The redshift adopted for the spectral model (Redshift)src.redshiftdoublelognHKLlog AGN column density, KL divergence (in nats units) (lognH_KL)stat.fit.paramdoubleB_lognHHlog AGN column density, HDI upper limit (lognH_HUp)log(cm**-2)phys.columnDensity;stat.maxdoublelogPowNKLlog power-law normalization, KL divergence (in nats units) (logPowNorm_KL)stat.fit.paramdoubleb_logPowNHlog power-law normalization, HDI lower limit (logPowNorm_HLo)log(ph.keV**-1.cm**-2.s**-1)arith.zp;arith.ratiodoubleB_logPowNHlog power-law normalization, HDI upper limit (logPowNorm_HUp)log(ph.keV**-1.cm**-2.s**-1)arith.zp;arith.ratiodoublelognHBFlog AGN column density, best-fit model (lognH_BF)log(cm**-2)phys.columnDensitydoublelogPowNBFlog power-law normalization, best-fit model (logPowNorm_BF)log(ph.keV**-1.cm**-2.s**-1)stat.fit.paramdoubleFluxObsBFSObserved flux in observed 0.5-2 keV, best-fit model (FluxObsv_BF_s)mW.m**-2phot.flux;em.X-raydoubleFluxObsMedSObserved flux in observed 0.5-2 keV, posterior median (FluxObsv_Med_s)mW.m**-2phot.flux;em.X-raydoubleb_FluxObsSObserved flux in observed 0.5-2 keV, 1sigma lower limit (FluxObsv_Lo1_s)mW.m**-2phot.flux;em.X-ray.softdoubleB_FluxObsSObserved flux in observed 0.5-2 keV, 1sigma upper limit (FluxObsv_Up1_s)mW.m**-2phot.flux;em.X-ray.softdoubleb2_FluxObsSObserved flux in observed 0.5-2 keV, 2sigma lower limit (FluxObsv_Lo2_s)mW.m**-2stat.errordoubleB2_FluxObsSObserved flux in observed 0.5-2 keV, 2sigma upper limit (FluxObsv_Up2_s)mW.m**-2stat.errordoubleFluxObsBFTObserved flux in observed 2.3-5 keV, best-fit model (FluxObsv_BF_t)mW.m**-2phot.flux;em.X-raydoubleFluxObsMedTObserved flux in observed 2.3-5 keV, posterior median (FluxObsv_Med_t)mW.m**-2phot.flux;em.X-raydoubleb_FluxObsTObserved flux in observed 2.3-5 keV, 1sigma lower limit (FluxObsv_Lo1)mW.m**-2phot.flux;em.X-ray.mediumdoubleB_FluxObsTObserved flux in observed 2.3-5 keV, 1sigma upper limit (FluxObsv_Up1)mW.m**-2phot.flux;em.X-ray.mediumdoubleb2_FluxObsTObserved flux in observed 2.3-5 keV, 2sigma lower limit (FluxObsv_Lo2)mW.m**-2stat.errordoubleB2_FluxObsTObserved flux in observed 2.3-5 keV, 2sigma upper limit (FluxObsv_Up2)mW.m**-2stat.errordoubleFluxCBFSAbsorption corrected flux in observed 0.5-2 keV, best-fit model (FluxCorr_BF_s)mW.m**-2phot.flux;em.X-raydoubleFluxCMedSAbsorption corrected flux in observed 0.5-2 keV, posterior median (FluxCorr_Med_s)mW.m**-2phot.flux;em.X-raydoubleb_FluxCSAbsorption corrected flux in observed 0.5-2 keV, 1sigma lower limit (FluxCorr_Lo1_s)mW.m**-2phot.flux;em.X-ray.softdoubleB_FluxCSAbsorption corrected flux in observed 0.5-2 keV, 1sigma upper limit (FluxCorr_Up1_s)mW.m**-2phot.flux;em.X-ray.softdoubleb2_FluxCSAbsorption corrected flux in observed 0.5-2 keV, 2sigma lower limit (FluxCorr_Lo2_s)mW.m**-2stat.errordoubleB2_FluxCSAbsorption corrected flux in observed 0.5-2 keV, 2sigma upper limit (FluxCorr_Up2_s)mW.m**-2stat.errordoubleFluxCBFTAbsorption corrected flux in observed 2.3-5 keV, best-fit model (FluxCorr_BF_t)mW.m**-2phot.flux;em.X-raydoubleFluxCMedTAbsorption corrected flux in observed 2.3-5 keV, posterior median (FluxCorr_Med_t)mW.m**-2phot.flux;em.X-raydoubleb_FluxCTAbsorption corrected flux in observed 2.3-5 keV, 1sigma lower limit (FluxCorr_Lo1)mW.m**-2phot.flux;em.X-ray.mediumdoubleB_FluxCTAbsorption corrected flux in observed 2.3-5 keV, 1sigma upper limit (FluxCorr_Up1)mW.m**-2phot.flux;em.X-ray.mediumdoubleb2_FluxCTAbsorption corrected flux in observed 2.3-5 keV, 2sigma lower limit (FluxCorr_Lo2)mW.m**-2stat.errordoubleB2_FluxCTAbsorption corrected flux in observed 2.3-5 keV, 2sigma upper limit (FluxCorr_Up2)mW.m**-2stat.errordoubleFluxIBFSAbsorption corrected flux in rest-frame 0.5-2 keV, best-fit model (FluxIntr_BF_s)mW.m**-2phot.flux;em.X-raydoubleFluxIMedSAbsorption corrected flux in rest-frame 0.5-2 keV, posterior median (FluxIntr_Med_s)mW.m**-2phot.flux;em.X-raydoubleb_FluxISAbsorption corrected flux in rest-frame 0.5-2keV, 1sigma lower limit (FluxIntr_Lo1_s)mW.m**-2phot.flux;em.X-ray.softdoubleB_FluxISAbsorption corrected flux in rest-frame 0.5-2keV, 1sigma upper limit (FluxIntr_Up1_s)mW.m**-2phot.flux;em.X-ray.softdoubleb2_FluxISAbsorption corrected flux in rest-frame 0.5-2 keV, 2sigma lower limit (FluxIntr_Lo2_s)mW.m**-2stat.errordoubleB2_FluxISAbsorption corrected flux in rest-frame 0.5-2 keV, 2sigma upper limit (FluxIntr_Up2_s)mW.m**-2stat.errordoubleFluxIBF2keVAbsorption corrected flux at rest-frame 2keV, best- fit (FluxIntr_BF_2keV)mW.m**-2.eV**-1phot.flux;em.X-raydoubleFluxIMed2keVAbsorption corrected flux at rest-frame 2keV, median (FluxIntr_Med_2keV)mW.m**-2.eV**-1phot.flux;em.X-raydoubleb_FluxI2keVAbsorption corrected flux at rest-frame 2keV, 1sigma lower limit (FluxIntr_Lo1_2keV)mW.m**-2.eV**-1phot.fluxdoubleB_FluxI2keVAbsorption corrected flux at rest-frame 2keV, 1sigma upper limit (FluxIntr_Up1_2keV)mW.m**-2.eV**-1phot.fluxdoubleb2_FluxI2keVAbsorption corrected flux at rest-frame 2keV, 2sigma lower limit (FluxIntr_Lo2_2keV)mW.m**-2.eV**-1stat.errordoubleB2_FluxI2keVAbsorption corrected flux at rest-frame 2keV, 2sigma upper limit (FluxIntr_Up2_2keV)mW.m**-2.eV**-1stat.errordoubleLumIBFS? Intrinsic luminosity in rest-frame 0.5-2 keV, best-fit model (LumiIntr_BF_s)1e-07Wphys.luminosity;em.X-raydoublenullableLumIMedS? Intrinsic luminosity in rest-frame 0.5-2 keV, posterior median (LumiIntr_Med_s)1e-07Wphys.luminosity;em.X-raydoublenullableb_LumIS? Intrinsic luminosity in rest-frame 0.5-2 keV, 1sigma lower limit (LumiIntr_Lo1_s)1e-07Wphys.luminosity;em.X-ray.softdoublenullableB_LumIS? Intrinsic luminosity in rest-frame 0.5-2 keV, 1sigma upper limit (LumiIntr_Up1_s)1e-07Wphys.luminosity;em.X-ray.softdoublenullableb2_LumIS? Intrinsic luminosity in rest-frame 0.5-2 keV, 2sigma lower limit (LumiIntr_Lo2_s)1e-07Wstat.errordoublenullableB2_LumIS? Intrinsic luminosity in rest-frame 0.5-2 keV, 2sigma upper limit (LumiIntr_Up2_s)1e-07Wstat.errordoublenullableLumIBF2keV? Intrinsic luminosity at rest-frame 2keV, best-fit model (LumiIntr_BF_2keV)1e-07W.eV**-1phys.luminosity;em.X-raydoublenullableLumIMed2keV? Intrinsic luminosity at rest-frame 2keV, posterior median (LumiIntr_Med_2keV)1e-07W.eV**-1phys.luminosity;em.X-raydoublenullableb2_LumI2keV? Intrinsic luminosity at rest-frame 2keV, 2sigma lower limit (LumiIntr_Lo2_2keV)1e-07W.eV**-1stat.errordoublenullableB2_LumI2keV? Intrinsic luminosity at rest-frame 2keV, 2sigma upper limit (LumiIntr_Up2_2keV)1e-07W.eV**-1stat.errordoublenullableb_lognHlog AGN column density, percentile lower limit (lognH_Lo)log(cm**-2)phys.columnDensity;stat.mindoubleB_lognHlog AGN column density, percentile upper limit (lognH_Up)log(cm**-2)phys.columnDensity;stat.maxdoublelognHMeanlog AGN column density, mean (lognH_Mean)log(cm**-2)phys.columnDensitydoubles_lognHlog AGN column density, standard deviation (lognH_Std)log(cm**-2)stat.stdev;phys.columnDensitydoublelogPowNMedlog power-law normalization, posterior median (logPowNorm_Med)log(ph.keV**-1.cm**-2.s**-1)stat.fit.paramdoubleb_logPowNlog power-law normalization, percentile lower limit (logPowNorm_Lo)log(ph.keV**-1.cm**-2.s**-1)arith.zp;arith.ratiodoubleB_logPowNlog power-law normalization, percentile upper limit (logPowNorm_Up)log(ph.keV**-1.cm**-2.s**-1)arith.zp;arith.ratiodoublelogPowNMeanlog power-law normalization, mean (logPowNorm_Mean)log(ph.keV**-1.cm**-2.s**-1)stat.fit.paramdoubles_logPowNlog power-law normalization, standard deviation (logPowNorm_Std)log(ph.keV**-1.cm**-2.s**-1)arith.zp;arith.ratiodoublelogBkgNMedlog background normalization, posterior median (logBkgNorm_Med)instr.backgrounddoubleb_logBkgNlog background normalization, percentile lower limit (logBkgNorm_Lo)instr.background;arith.ratiodoubleB_logBkgNlog background normalization, percentile upper limit (logBkgNorm_Up)instr.background;arith.ratiodoublelogBkgNMeanlog background normalization, mean (logBkgNorm_Mean)instr.backgrounddoubles_logBkgNlog background normalization, standard deviation (logBkgNorm_Std)instr.background;arith.ratiodoublelogZlog10 Bayesian evidence (logZ)stat.fit.paramdoublePaperIDisplay the Paper I (Brunner et al., Cat. J/A+A/661/A1) datameta.ref.urlcharPaperIIDisplay the Paper II (Salvato et al., Cat. J/A+A/661/A3) datameta.ref.urlcharJ/A+A/661/A5/table8Shape-fixed-powerlaw resultsFluxObsMedSObserved flux in observed 0.5-2 keV, posterior median (FluxObsv_Med_s)mW.m**-2phot.flux;em.X-raydoubleFluxIBF2keVAbsorption corrected flux at rest-frame 2keV, best- fit (FluxIntr_BF_2keV)mW.m**-2.eV**-1phot.flux;em.X-raydoublePaperIIDisplay the Paper II (Salvato et al., Cat. J/A+A/661/A3) datameta.ref.urlcharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintID-SRC[1/32683] ID of the sources in the eFEDS main X-ray catalog (Paper I) (ID_SRC)meta.id;meta.mainintz[-0.01/8.0] The redshift adopted for the spectral model (Redshift)src.redshiftdoublelogPowNKLlog power-law normalization, KL divergence (in nats units) (logPowNorm_KL)stat.fit.paramdoubleb_logPowNHlog power-law normalization, HDI lower limit (logPowNorm_HLo)log(ph.keV**-1.cm**-2.s**-1)arith.zp;arith.ratiodoubleB_logPowNHlog power-law normalization, HDI upper limit (logPowNorm_HUp)log(ph.keV**-1.cm**-2.s**-1)arith.zp;arith.ratiodoublelogPowNBFlog power-law normalization, best-fit model (logPowNorm_BF)log(ph.keV**-1.cm**-2.s**-1)stat.fit.paramdoubleFluxObsBFSObserved flux in observed 0.5-2 keV, best-fit model (FluxObsv_BF_s)mW.m**-2phot.flux;em.X-raydoubleb_FluxObsSObserved flux in observed 0.5-2 keV, 1sigma lower limit (FluxObsv_Lo1_s)mW.m**-2phot.flux;em.X-ray.softdoubleB_FluxObsSObserved flux in observed 0.5-2 keV, 1sigma upper limit (FluxObsvs)mW.m**-2phot.flux;em.X-ray.softdoubleb2_FluxObsSObserved flux in observed 0.5-2 keV, 2sigma lower limit (FluxObsvs)mW.m**-2stat.errordoubleB2_FluxObsSObserved flux in observed 0.5-2 keV, 2sigma upper limit (FluxObsvs)mW.m**-2stat.errordoubleFluxObsBFTObserved flux in observed 2.3-5 keV, best-fit model (FluxObsv_BF_t)mW.m**-2phot.flux;em.X-raydoubleFluxObsMedTObserved flux in observed 2.3-5 keV, posterior median (FluxObsv_Med_t)mW.m**-2phot.flux;em.X-raydoubleb_FluxObsTObserved flux in observed 2.3-5 keV, 1sigma lower limit (FluxObsv_Lo1_t)mW.m**-2phot.flux;em.X-ray.mediumdoubleB_FluxObsTObserved flux in observed 2.3-5 keV, 1sigma upper limit (FluxObsvt)mW.m**-2phot.flux;em.X-ray.mediumdoubleb2_FluxObsTObserved flux in observed 2.3-5 keV, 2sigma lower limit (FluxObsvt)mW.m**-2stat.errordoubleB2_FluxObsTObserved flux in observed 2.3-5 keV, 2sigma upper limit (FluxObsvt)mW.m**-2stat.errordoubleFluxCBFSAbsorption corrected flux in observed 0.5-2 keV, best-fit model (FluxCorr_BF_s)mW.m**-2phot.flux;em.X-raydoubleFluxCMedSAbsorption corrected flux in observed 0.5-2 keV, posterior median (FluxCorr_Med_s)mW.m**-2phot.flux;em.X-raydoubleb_FluxCSAbsorption corrected flux in observed 0.5-2 keV, 1sigma lower limit (FluxCorr_Lo1_s)mW.m**-2phot.flux;em.X-ray.softdoubleB_FluxCSAbsorption corrected flux in observed 0.5-2 keV, 1sigma upper limit (FluxCorrs)mW.m**-2phot.flux;em.X-ray.softdoubleb2_FluxCSAbsorption corrected flux in observed 0.5-2 keV, 2sigma lower limit (FluxCorrs)mW.m**-2stat.errordoubleB2_FluxCSAbsorption corrected flux in observed 0.5-2 keV, 2sigma upper limit (FluxCorrs)mW.m**-2stat.errordoubleFluxCBFTAbsorption corrected flux in observed 2.3-5 keV, best-fit model (FluxCorr_BF_t)mW.m**-2phot.flux;em.X-raydoubleFluxCMedTAbsorption corrected flux in observed 2.3-5 keV, posterior median (FluxCorr_Med_t)mW.m**-2phot.flux;em.X-raydoubleb_FluxCTAbsorption corrected flux in observed 2.3-5 keV, 1sigma lower limit (FluxCorr_Lo1_t)mW.m**-2phot.flux;em.X-ray.mediumdoubleB_FluxCTAbsorption corrected flux in observed 2.3-5 keV, 1sigma upper limit (FluxCorrt)mW.m**-2phot.flux;em.X-ray.mediumdoubleb2_FluxCTAbsorption corrected flux in observed 2.3-5 keV, 2sigma lower limit (FluxCorrt)mW.m**-2stat.errordoubleB2_FluxCTAbsorption corrected flux in observed 2.3-5 keV, 2sigma upper limit (FluxCorrt)mW.m**-2stat.errordoubleFluxIBFSAbsorption corrected flux in rest-frame 0.5-2 keV, best-fit model (FluxIntr_BF_s)mW.m**-2phot.flux;em.X-raydoubleFluxIMedSAbsorption corrected flux in rest-frame 0.5-2 keV, posterior median (FluxIntr_Med_s)mW.m**-2phot.flux;em.X-raydoubleb_FluxISAbsorption corrected flux in rest-frame 0.5-2keV, 1sigma lower limit (FluxIntr_Lo1_s)mW.m**-2phot.flux;em.X-ray.softdoubleB_FluxISAbsorption corrected flux in rest-frame 0.5-2keV, 1sigma upper limit (FluxIntrs)mW.m**-2phot.flux;em.X-ray.softdoubleb2_FluxISAbsorption corrected flux in rest-frame 0.5-2 keV, 2sigma lower limit (FluxIntrs)mW.m**-2stat.errordoubleB2_FluxISAbsorption corrected flux in rest-frame 0.5-2 keV, 2sigma upper limit (FluxIntrs)mW.m**-2stat.errordoubleFluxIMed2keVAbsorption corrected flux at rest-frame 2keV, median (FluxIntr_Med_2keV)mW.m**-2.eV**-1phot.flux;em.X-raydoubleb_FluxI2keVAbsorption corrected flux at rest-frame 2keV, 1sigma lower limit (FluxIntr_Lo1_2keV)mW.m**-2.eV**-1phot.fluxdoubleB_FluxI2keVAbsorption corrected flux at rest-frame 2keV, 1sigma upper limit (FluxIntr_Up1_2keV)mW.m**-2.eV**-1phot.fluxdoubleb2_FluxI2keVAbsorption corrected flux at rest-frame 2keV, 2sigma lower limit (FluxIntr_Lo2_2keV)mW.m**-2.eV**-1stat.errordoubleB2_FluxI2keVAbsorption corrected flux at rest-frame 2keV, 2sigma upper limit (FluxIntr_Up2_2keV)mW.m**-2.eV**-1stat.errordoubleLumIBFS? Intrinsic luminosity in rest-frame 0.5-2 keV, best-fit model (LumiIntr_BF_s)1e-07Wphys.luminosity;em.X-raydoublenullableLumIMedS? Intrinsic luminosity in rest-frame 0.5-2 keV, posterior median (LumiIntr_Med_s)1e-07Wphys.luminosity;em.X-raydoublenullableb_LumIS? Intrinsic luminosity in rest-frame 0.5-2 keV, 1sigma lower limit (LumiIntr_Lo1_s)1e-07Wphys.luminosity;em.X-ray.softdoublenullableB_LumIS? Intrinsic luminosity in rest-frame 0.5-2 keV, 1sigma upper limit (LumiIntrs)1e-07Wphys.luminosity;em.X-ray.softdoublenullableb2_LumI2S? Intrinsic luminosity in rest-frame 0.5-2 keV, 2sigma lower limit (LumiIntrs)1e-07Wstat.errordoublenullableB2_LumIS? Intrinsic luminosity in rest-frame 0.5-2 keV, 2sigma upper limit (LumiIntrs)1e-07Wstat.errordoublenullableLumIBF2keV? Intrinsic luminosity at rest-frame 2keV, best-fit model (LumiIntr_BF_2keV)1e-07W.eV**-1phys.luminosity;em.X-raydoublenullableLumIMed2keV? Intrinsic luminosity at rest-frame 2keV, posterior median (LumiIntr_Med_2keV)1e-07W.eV**-1phys.luminosity;em.X-raydoublenullableb_LumI2keV? Intrinsic luminosity at rest-frame 2keV, 1sigma lower limit (LumiIntr_Lo1_2keV)1e-07W.eV**-1phys.luminositydoublenullableB_LumI2keV? Intrinsic luminosity at rest-frame 2keV, 1sigma upper limit (LumiIntr_Up1_2keV)1e-07W.eV**-1phys.luminositydoublenullableb2_LumI2keV? Intrinsic luminosity at rest-frame 2keV, 2sigma lower limit (LumiIntr_Lo2_2keV)1e-07W.eV**-1stat.errordoublenullableB2_LumI2keV? Intrinsic luminosity at rest-frame 2keV, 2sigma upper limit (LumiIntr_Up2_2keV)1e-07W.eV**-1stat.errordoublenullablelogPowNMedlog power-law normalization, posterior median (logPowNorm_Med)log(ph.keV**-1.cm**-2.s**-1)stat.fit.paramdoubleb_logPowNlog power-law normalization, percentile lower limit (logPowNorm_Lo)log(ph.keV**-1.cm**-2.s**-1)arith.zp;arith.ratiodoubleB_logPowNlog power-law normalization, percentile upper limit (logPowNorm_Up)log(ph.keV**-1.cm**-2.s**-1)arith.zp;arith.ratiodoublelogPowNMeanlog power-law normalization, mean (logPowNorm_Mean)log(ph.keV**-1.cm**-2.s**-1)stat.fit.paramdoubles_logPowNlog power-law normalization, standard deviation (logPowNorm_Std)log(ph.keV**-1.cm**-2.s**-1)arith.zp;arith.ratiodoublelogBkgNMedlog background normalization, posterior median (logBkgNorm_Med)instr.backgrounddoubleb_logBkgNlog background normalization, percentile lower limit (logBkgNorm_Lo)instr.background;arith.ratiodoubleB_logBkgNlog background normalization, percentile upper limit (logBkgNorm_Up)instr.background;arith.ratiodoublelogBkgNMeanlog background normalization, mean (logBkgNorm_Mean)instr.backgrounddoubles_logBkgNlog background normalization, standard deviation (logBkgNorm_Std)instr.background;arith.ratiodoublelogZlog10 Bayesian evidence (logZ)stat.fit.paramdoublePaperIDisplay the Paper I (Brunner et al., Cat. J/A+A/661/A1) datameta.ref.urlcharJ/A+A/661/A5/table9Soft-band fitting resultsb_GammaHpower-law slope, HDI lower limit (Gamma_HLo)arith.grad;stat.mindoubleb_logPowNlog power-law normalization, percentile lower limit (logPowNorm_Lo)log(ph.keV**-1.cm**-2.s**-1)arith.zp;arith.ratiodoubleB_logPowNlog power-law normalization, percentile upper limit (logPowNorm_Up)log(ph.keV**-1.cm**-2.s**-1)arith.zp;arith.ratiodoublelogBkgNMedlog background normalization, posterior median (logBkgNorm_Med)instr.backgrounddoublerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintID-SRC[1/32683] ID of the sources in the eFEDS main X-ray catalog (Paper I) (ID_SRC)meta.id;meta.mainintz[-0.01/8.0] The redshift adopted for the spectral model (Redshift)src.redshiftdoubleGammaKLpower-law slope, KL divergence (in nats units) (Gamma_KL)stat.fit.paramdoubleB_GammaHpower-law slope, HDI upper limit (Gamma_HUp)arith.grad;stat.maxdoublelognHKLlog AGN column density, KL divergence (in nats units) (lognH_KL)stat.fit.paramdoubleb_lognHHlog AGN column density, HDI lower limit (lognH_HLo)log(cm**-2)phys.columnDensity;stat.mindoubleB_lognHHlog AGN column density, HDI upper limit (lognH_HUp)log(cm**-2)phys.columnDensity;stat.maxdoublelogPowNKLlog power-law normalization, KL divergence (in nats units) (logPowNorm_KL)stat.fit.paramdoubleb_logPowNHlog power-law normalization, HDI lower limit (logPowNorm_HLo)log(ph.keV**-1.cm**-2.s**-1)arith.zp;arith.ratiodoubleB_logPowNHlog power-law normalization, HDI upper limit (logPowNorm_HUp)log(ph.keV**-1.cm**-2.s**-1)arith.zp;arith.ratiodoubleGammaBFpower-law slope, best-fit model (Gamma_BF)spect.indexdoublelognHBFlog AGN column density, best-fit model (lognH_BF)log(cm**-2)phys.columnDensitydoublelogPowNBFlog power-law normalization, best-fit model (logPowNorm_BF)log(ph.keV**-1.cm**-2.s**-1)stat.fit.paramdoubleFluxObsBFSObserved flux in observed 0.5-2 keV, best-fit model (FluxObsv_BF_s)mW.m**-2phot.flux;em.X-raydoubleFluxObsMedSObserved flux in observed 0.5-2 keV, posterior median (FluxObsv_Med_s)mW.m**-2phot.flux;em.X-raydoubleb_FluxObsSObserved flux in observed 0.5-2 keV, 1sigma lower limit (FluxObsv_Lo1_s)mW.m**-2phot.flux;em.X-ray.softdoubleB_FluxObsSObserved flux in observed 0.5-2 keV, 1sigma upper limit (FluxObsv_Up1_s)mW.m**-2phot.flux;em.X-ray.softdoubleb2_FluxObsSObserved flux in observed 0.5-2 keV, 2sigma lower limit (FluxObsv_Lo2_s)mW.m**-2phot.flux;em.X-raydoubleB2_FluxObsSObserved flux in observed 0.5-2 keV, 2sigma upper limit (FluxObsv_Up2_s)mW.m**-2phot.flux;em.X-raydoubleGammaMedpower-law slope, posterior median (Gamma_Med)spect.indexdoubleb_Gammapower-law slope, percentile lower limit (Gamma_Lo)arith.grad;stat.mindoubleB_Gammapower-law slope, percentile upper limit (Gamma_Up)arith.grad;stat.maxdoubleGammaMeanpower-law slope, mean (Gamma_Mean)spect.indexdoubles_Gammapower-law slope, standard deviation (Gamma_Std)stat.stdevdoublelognHMedlog AGN column density, posterior median (lognH_Med)log(cm**-2)phys.columnDensitydoubleb_lognHlog AGN column density, percentile lower limit (lognH_Lo)log(cm**-2)phys.columnDensity;stat.mindoubleB_lognHlog AGN column density, percentile upper limit (lognH_Up)log(cm**-2)phys.columnDensity;stat.maxdoublelognHMeanlog AGN column density, mean (lognH_Mean)log(cm**-2)phys.columnDensitydoubles_lognHlog AGN column density, standard deviation (lognH_Std)log(cm**-2)stat.stdev;phys.columnDensitydoublelogPowNMedlog power-law normalization, posterior median (logPowNorm_Med)log(ph.keV**-1.cm**-2.s**-1)stat.fit.paramdoublelogPowNMeanlog power-law normalization, mean (logPowNorm_Mean)log(ph.keV**-1.cm**-2.s**-1)stat.fit.paramdoubles_logPowNlog power-law normalization, standard deviation (logPowNorm_Std)log(ph.keV**-1.cm**-2.s**-1)arith.zp;arith.ratiodoubleblogBkgNlog background normalization, percentile lower limit (logBkgNorm_Lo)stat.errordoubleBlogBkgNlog background normalization, percentile upper limit (logBkgNorm_Up)stat.errordoublelogBkgNMeanlog background normalization, mean (logBkgNorm_Mean)instr.backgrounddoublelogBkgNlog background normalization, standard deviation (logBkgNorm_Std)instr.backgrounddoublelogZlog10 Bayesian evidence (logZ)stat.fit.paramdoublePaperIDisplay the Paper I (Brunner et al., Cat. J/A+A/661/A1) datameta.ref.urlcharPaperIIDisplay the Paper II (Salvato et al., Cat. J/A+A/661/A3) datameta.ref.urlcharJ/A+A/661/A5/table10Hard-band fitting resultsGammaMedpower-law slope, posterior median (Gamma_Med)spect.indexdoubleb_GammaMedpower-law slope, percentile lower limit (Gamma_Lo)arith.grad;stat.mindoubleB_GammaMedpower-law slope, percentile upper limit (Gamma_Up)arith.grad;stat.maxdoublerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintID-SRC[1/32683] ID of the sources in the eFEDS main X-ray catalog (Paper I) (ID_SRC)meta.id;meta.mainintz[-0.01/8.0] The redshift adopted for the spectral model (Redshift)src.redshiftdoubleGammaKLpower-law slope, KL divergence (in nats units) (Gamma_KL)stat.fit.paramdoublee_Gammapower-law slope, HDI lower limit (Gamma_HLo)stat.errordoubleE_Gammapower-law slope, HDI upper limit (Gamma_HUp)stat.error;stat.maxdoublelognHKLlog AGN column density, KL divergence (in nats units) (lognH_KL)stat.fit.paramdoubleb_lognHlog AGN column density, HDI lower limit (lognH_HLo)log(cm**-2)phys.columnDensity;stat.mindoubleB_lognHlog AGN column density, HDI upper limit (lognH_HUp)log(cm**-2)phys.columnDensity;stat.maxdoublelogPowNKLlog power-law normalization, KL divergence (in nats units) (logPowNorm_KL)stat.fit.paramdoubleb_logPowNlog power-law normalization, HDI lower limit (logPowNorm_HLo)log(ph.keV**-1.cm**-2.s**-1)arith.zp;arith.ratiodoubleB_logPowNlog power-law normalization, HDI upper limit (logPowNorm_HUp)log(ph.keV**-1.cm**-2.s**-1)arith.zp;arith.ratiodoubleGammaBFpower-law slope, best-fit model (Gamma_BF)spect.indexdoublelognHBFlog AGN column density, best-fit model (lognH_BF)log(cm**-2)phys.columnDensitydoublelogPowNBFlog power-law normalization, best-fit model (logPowNorm_BF)log(ph.keV**-1.cm**-2.s**-1)stat.fit.paramdoubleFluxObsBFTObserved flux in observed 2.3-5keV, best-fit model (FluxObsv_BF_t)mW.m**-2phot.flux;em.X-raydoubleFluxObsMedTObserved flux in observed 2.3-5keV, posterior median (FluxObsv_Med_t)mW.m**-2phot.flux;em.X-raydoubleb_FluxObsTObserved flux in observed 2.3-5keV, 1sigma lower limit (FluxObsv_Lo1_t)mW.m**-2phot.flux;em.X-ray.mediumdoubleB_FluxObsTObserved flux in observed 2.3-5keV, 1sigma upper limit (FluxObsv_Up1_t)mW.m**-2phot.flux;em.X-ray.mediumdoubleb2_FluxObsTObserved flux in observed 2.3-5keV, 2sigma lower limit (FluxObsv_Lo2_t)mW.m**-2stat.errordoubleB2_FluxObsTObserved flux in observed 2.3-5keV, 2sigma upper limit (FluxObsv_Up2_t)mW.m**-2stat.errordoubleFluxCBFTAbsorption corrected flux in observed 2.3-5 keV, best-fit model (FluxCorr_BF_t)mW.m**-2phot.flux;em.X-raydoubleFluxCMedTAbsorption corrected flux in observed 2.3-5 keV, posterior median (FluxCorr_Med_t)mW.m**-2phot.flux;em.X-raydoubleb_FluxCMedTAbsorption corrected flux in observed 2.3-5 keV, 1sigma lower limit (FluxCorr_Lo1_t)mW.m**-2phot.flux;em.X-ray.mediumdoubleB_FluxCMedTAbsorption corrected flux in observed 2.3-5 keV, 1sigma upper limit (FluxCorr_Up1_t)mW.m**-2phot.flux;em.X-ray.mediumdoubleb2_FluxCMedTAbsorption corrected flux in observed 2.3-5 keV, 2sigma lower limit (FluxCorr_Lo2_t)mW.m**-2stat.errordoubleB2_FluxCMedTAbsorption corrected flux in observed 2.3-5 keV, 2sigma upper limit (FluxCorr_Up2_t)mW.m**-2stat.errordoubleGammaMeanpower-law slope, mean (Gamma_Mean)spect.indexdoubles_Gammapower-law slope, standard deviation (Gamma_Std)stat.stdevdoublelognHMedlog AGN column density, posterior median (lognH_Med)log(cm**-2)phys.columnDensitydoubleb_lognHMedlog AGN column density, percentile lower limit (lognH_Lo)log(cm**-2)phys.columnDensity;stat.mindoubleB_lognHMedlog AGN column density, percentile upper limit (lognH_Up)log(cm**-2)phys.columnDensity;stat.maxdoublelognHMeanlog AGN column density, mean (lognH_Mean)log(cm**-2)phys.columnDensitydoubles_lognHlog AGN column density, standard deviation (lognH_Std)log(cm**-2)stat.stdev;phys.columnDensitydoublelogPowNMedlog power-law normalization, posterior median (logPowNorm_Med)log(ph.keV**-1.cm**-2.s**-1)stat.fit.paramdoubleb_logPowNMedlog power-law normalization, percentile lower limit (logPowNorm_Lo)log(ph.keV**-1.cm**-2.s**-1)arith.zp;arith.ratiodoubleB_logPowNMedlog power-law normalization, percentile upper limit (logPowNorm_Up)log(ph.keV**-1.cm**-2.s**-1)arith.zp;arith.ratiodoublelogPowNMeanlog power-law normalization, mean (logPowNorm_Mean)log(ph.keV**-1.cm**-2.s**-1)stat.fit.paramdoubles_logPowNlog power-law normalization, standard deviation (logPowNorm_Std)log(ph.keV**-1.cm**-2.s**-1)arith.zp;arith.ratiodoublelogBkgNMedlog background normalization, posterior median (logBkgNorm_Med)instr.backgrounddoubleb_logBkgNMedlog background normalization, percentile lower limit (logBkgNorm_Lo)instr.background;arith.ratiodoubleB_logBkgNMedlog background normalization, percentile upper limit (logBkgNorm_Up)instr.background;arith.ratiodoublelogBkgNMeanlog background normalization, mean (logBkgNorm_Mean)instr.backgrounddoubles_logBkgNlog background normalization, standard deviation (logBkgNorm_Std)instr.background;arith.ratiodoublelogZlog10 Bayesian evidence (logZ)stat.fit.paramdoublePaperIDisplay the Paper I (Brunner et al., Cat. J/A+A/661/A1) datameta.ref.urlcharPaperIIDisplay the Paper II (Salvato et al., Cat. J/A+A/661/A3) datameta.ref.urlchar