eFEDS AGN catalog and X-ray spectral properties

NOTE: new version (V17.3) released in Feb. 2022!

General Description

The eFEDS AGN catalog and X-ray spectral fitting results of all the eFEDS sources.

Approximate Size

62 MB

File Type

FITS

Generated by Product

eSASS

Xspec 12.11

BXA 4.0.2

Sections

• The eFEDS AGN catalog
• Basic X-ray spectral properties of eFEDS sources
• Spectral fitting results with model 0: APEC
• Spectral fitting results with model 1: single-powerlaw
• Spectral fitting results with model 2: double-powerlaw
• Spectral fitting results with model 3: power-law plus blackbody
• Spectral fitting results with model 4: Gamma-fixed-powerlaw
• Spectral fitting results with model 5: shape-fixed-powerlaw
• Spectral fitting results with model 6: soft-band fitting
• Spectral fitting results with model 7: hard-band fitting
• References
• Acknowledgement

The eFEDS AGN catalog

The eFEDS AGN catalog

Binary Table Caption for HDU1

Name	Type	Unit	Description
ID_SRC	int32[1]		ID of the sources in the eFEDS main X-ray catalog (Paper I)
RA_CORR	float64[1]	deg	Right ascension (J2000), astrometric corrected (Paper I)
DEC_CORR	float64[1]	deg	Declination (J2000), astrometric corrected (Paper I)
DET_LIKE	float32		0.2-2.3 keV source detection likelihood (Paper I)
inArea90	bool[1]		Whether located inside the inner 90%-area region of eFEDS (Paper I)
CTP_LS8_UNIQUE_OBJID	char[11]		ID of the best LS8 counterpart (Paper II)
CTP_LS8_RA	float64	deg	Right ascension (J2000) of the best LS8 counterpart (Paper II)
CTP_LS8_Dec	float64	deg	Declination (J2000) of the best LS8 counterpart (Paper II)
CTP_quality	int16		Counterpart quality (Paper II). A value ≥2 is recommended.
CTP_CLASS	int16		Classification of the optical counterpart (Paper II). 0:likely Galactic; 1:secure Galac.; 2:likely extraGalactic; 3:secure extraGalac.
CTP_REDSHIFT	float64		Redshift of the optical counterpart (Paper II)
CTP_REDSHIFT_GRADE	int32[1]		Redshift Grade (Paper II). A value ≥3 is recommended.
in_KiDS_flag	bool		Whether located inside the region of the KiDS survey (Paper II)
Model	int32[1]		Index of selected model for luminosity measurement. 1:single-powerlaw; 2:double-powerlaw; 4:powerlaw with Gamma 2.0; 5:shape-fixed
NHclass	int32[1]		Class of AGN NH measurement with model 1 (single-powerlaw). 1: uninformative; 2: unobscured; 3: mildly-measured; 4: well-measured
FSclass	int32[1]		Class of 0.5-2 keV flux measurement. 0:model 5 (shape-fixed; faintest); 1:m2(double-powerlaw); 2:m6(0.4-2.2keV fit); 3:m0(APEC; stars)
FHclass	int32[1]		Class of 2.3-5 keV flux measurement. 0: model 5 (shape-fixed powerlaw; for faintest sources); 1: model 7 (powerlaw fitting in 2.3-6 keV)
galNH	float64	cm^-2	Galactic absorption column density from HI4PI
FluxCorr_BF_s	float32	erg/cm^2/s	Absorption corrected flux in observed 0.5-2 keV, best-fit model
FluxCorr_Med_s	float32	erg/cm^2/s	Absorption corrected flux in observed 0.5-2 keV, posterior median
FluxCorr_Lo1_s	float32	erg/cm^2/s	Absorption corrected flux in observed 0.5-2 keV, 1sigma lower limit
FluxCorr_Up1_s	float32	erg/cm^2/s	Absorption corrected flux in observed 0.5-2 keV, 1sigma upper limit
FluxCorr_Lo2_s	float32	erg/cm^2/s	Absorption corrected flux in observed 0.5-2 keV, 2sigma lower limit
FluxCorr_Up2_s	float32	erg/cm^2/s	Absorption corrected flux in observed 0.5-2 keV, 2sigma upper limit
FluxCorr_BF_t	float32	erg/cm^2/s	Absorption corrected flux in observed 2.3-5 keV, best-fit model
FluxCorr_Med_t	float32	erg/cm^2/s	Absorption corrected flux in observed 2.3-5 keV, posterior median
FluxCorr_Lo1_t	float32	erg/cm^2/s	Absorption corrected flux in observed 2.3-5 keV, 1sigma lower limit
FluxCorr_Up1_t	float32	erg/cm^2/s	Absorption corrected flux in observed 2.3-5 keV, 1sigma upper limit
FluxCorr_Lo2_t	float32	erg/cm^2/s	Absorption corrected flux in observed 2.3-5 keV, 2sigma lower limit
FluxCorr_Up2_t	float32	erg/cm^2/s	Absorption corrected flux in observed 2.3-5 keV, 2sigma upper limit
FluxIntr_BF_s	float32	erg/cm^2/s	Absorption corrected flux in rest-frame 0.5-2 keV, best-fit model
FluxIntr_Med_s	float32	erg/cm^2/s	Absorption corrected flux in rest-frame 0.5-2 keV, posterior median
FluxIntr_Lo1_s	float32	erg/cm^2/s	Absorption corrected flux in rest-frame 0.5-2keV, 1sigma lower limit
FluxIntr_Up1_s	float32	erg/cm^2/s	Absorption corrected flux in rest-frame 0.5-2keV, 1sig upper limit
FluxIntr_Lo2_s	float32	erg/cm^2/s	Absorption corrected flux in rest-frame 0.5-2 keV, 2sig lower limit
FluxIntr_Up2_s	float32	erg/cm^2/s	Absorption corrected flux in rest-frame 0.5-2 keV, 2sig upper limit
FluxIntr_BF_h	float32	erg/cm^2/s	Absorption corrected flux in rest-frame 2-10 keV, best-fit model
FluxIntr_Med_h	float32	erg/cm^2/s	Absorption corrected flux in rest-frame 2-10 keV, posterior median
FluxIntr_Lo1_h	float32	erg/cm^2/s	Absorption corrected flux in rest-frame 2-10 keV, 1sigma lower limit
FluxIntr_Up1_h	float32	erg/cm^2/s	Absorption corrected flux in rest-frame 2-10 keV, 1sigma upper limit
FluxIntr_Lo2_h	float32	erg/cm^2/s	Absorption corrected flux in rest-frame 2-10 keV, 2sigma lower limit
FluxIntr_Up2_h	float32	erg/cm^2/s	Absorption corrected flux in rest-frame 2-10 keV, 2sigma upper limit
FluxIntr_BF_2keV	float32	erg/cm^2/s	Absorption corrected flux in rest-frame 1.999-2.001 keV, best-fit
FluxIntr_Med_2keV	float32	erg/cm^2/s	Absorption corrected flux in rest-frame 1.999-2.001 keV, median
FluxIntr_Lo1_2keV	float32	erg/cm^2/s	Absorption corrected flux in rest-f. 1.999-2.001keV, 1sig lowerlimit
FluxIntr_Up1_2keV	float32	erg/cm^2/s	Absorption corrected flux in rest-f. 1.999-2.001keV, 1sig upperlimit
FluxIntr_Lo2_2keV	float32	erg/cm^2/s	Absorption corrected flux in rest-f. 1.999-2.001keV, 2sig lowerlimit
FluxIntr_Up2_2keV	float32	erg/cm^2/s	Absorption corrected flux in rest-f. 1.999-2.001keV, 2sig upperlimit
LumiIntr_BF_s	float32	erg/s	Intrinsic luminosity in rest-frame 0.5-2 keV, best-fit model
LumiIntr_Med_s	float32	erg/s	Intrinsic luminosity in rest-frame 0.5-2 keV, posterior median
LumiIntr_Lo1_s	float32	erg/s	Intrinsic luminosity in rest-frame 0.5-2 keV, 1sigma lower limit
LumiIntr_Up1_s	float32	erg/s	Intrinsic luminosity in rest-frame 0.5-2 keV, 1sigma upper limit
LumiIntr_Lo2_s	float32	erg/s	Intrinsic luminosity in rest-frame 0.5-2 keV, 2sigma lower limit
LumiIntr_Up2_s	float32	erg/s	Intrinsic luminosity in rest-frame 0.5-2 keV, 2sigma upper limit
LumiIntr_BF_h	float32	erg/s	Intrinsic luminosity in rest-frame 2-10 keV, best-fit model
LumiIntr_Med_h	float32	erg/s	Intrinsic luminosity in rest-frame 2-10 keV, posterior median
LumiIntr_Lo1_h	float32	erg/s	Intrinsic luminosity in rest-frame 2-10 keV, 1sigma lower limit
LumiIntr_Up1_h	float32	erg/s	Intrinsic luminosity in rest-frame 2-10 keV, 1sigma upper limit
LumiIntr_Lo2_h	float32	erg/s	Intrinsic luminosity in rest-frame 2-10 keV, 2sigma lower limit
LumiIntr_Up2_h	float32	erg/s	Intrinsic luminosity in rest-frame 2-10 keV, 2sigma upper limit
LumiIntr_BF_2keV	float32	erg/s	Intrinsic luminosity in rest-frame 1.999-2.001 keV, best-fit model
LumiIntr_Med_2keV	float32	erg/s	Intrinsic luminosity in rest-frame 1.999-2.001 keV, posterior median
LumiIntr_Lo1_2keV	float32	erg/s	Intrinsic luminosity in rest-frame 1.999-2.001 keV, 1sig lower limit
LumiIntr_Up1_2keV	float32	erg/s	Intrinsic luminosity in rest-frame 1.999-2.001 keV, 1sig upper limit
LumiIntr_Lo2_2keV	float32	erg/s	Intrinsic luminosity in rest-frame 1.999-2.001 keV, 2sig lower limit
LumiIntr_Up2_2keV	float32	erg/s	Intrinsic luminosity in rest-frame 1.999-2.001 keV, 2sig upper limit
FluxObsv_Med_s	float32	erg/cm^2/s	Observed flux in observed 0.5-2 keV, posterior median
FluxObsv_Lo1_s	float32	erg/cm^2/s	Observed flux in observed 0.5-2 keV, 1sigma lower limit
FluxObsv_Up1_s	float32	erg/cm^2/s	Observed flux in observed 0.5-2 keV, 1sigma upper limit
FluxObsv_Med_t	float32	erg/cm^2/s	Observed flux in observed 2.3-5 keV, posterior median
FluxObsv_Lo1_t	float32	erg/cm^2/s	Observed flux in observed 2.3-5 keV, 1sigma lower limit
FluxObsv_Up1_t	float32	erg/cm^2/s	Observed flux in observed 2.3-5 keV, 1sigma upper limit
lognH_KL_m1	float32	nats	log AGN column density, KL divergence
lognH_HLo_m1	float32	cm^-2	log AGN column density, HDI lower limit
lognH_HUp_m1	float32	cm^-2	log AGN column density, HDI upper limit
lognH_Med_m1	float32	cm^-2	log AGN column density, posterior median
Gamma_KL_m2	float32	nats	power-law slope, KL divergence
Gamma_HLo_m2	float32		power-law slope, HDI lower limit
Gamma_HUp_m2	float32		power-law slope, HDI upper limit
Gamma_Med_m2	float32		power-law slope, posterior median
logZ_m0	float32[1]		log Bayesian evidence with model 0: APEC
logZ_m1	float32[1]		log Bayesian evidence with model 1: single powerlaw
logZ_m2	float32		log Bayesian evidence with model 2: double powerlaw
logZ_m3	float32		log Bayesian evidence with model 3: powerlaw + blackbody
logZ_m4	float32[1]		log Bayesian evidence with model 4: powerlaw with Gamma fixed at 2.0
logZ_m5	float32[1]		log Bayesian evidence with model 5: shape-fixed powerlaw
L2500	float32	erg/s/Hz	The rest-frame 2500 luminosity in erg/s/Hz
L5100	float32	erg/s/Hz	The rest-frame 5100 luminosity in erg/s/Hz
W1	float32	ABmag	LS8-WISE W1 AB magnitude (Paper II)
W1_ERR	float32	ABmag	LS8-WISE W1 magnitude error (Paper II)
W2	float32	ABmag	LS8-WISE W2 AB magnitude (Paper II)
W2_ERR	float32	ABmag	LS8-WISE W2 magnitude error (Paper II)

Basic X-ray spectral properties of eFEDS sources

For all the sources in the eFEDS main catalog, we present spectra extraction information, count rates, and observed fluxes.

Binary Table Caption for HDU1

Name	Type	Unit	Description
ID_SRC	int32		ID of the sources in the eFEDS main X-ray catalog (Paper I)
RA_CORR	float64[1]	deg	Right ascension (J2000), astrometric corrected (Paper I)
DEC_CORR	float64[1]	deg	Declination (J2000), astrometric corrected (Paper I)
DET_LIKE	float32		0.2-2.3 keV source detection likelihood (Paper I)
inArea90	bool[1]		Whether located inside the inner 90%-area region of eFEDS (Paper I)
galNH	float64	cm^-2	Galactic absorption column density from HI4PI
Exposure	float32	seconds	Spectra exposure time
SrcCts	float32[1]	counts	Source net counts in the 0.2-5 keV band
RA	float32	deg	Right ascension (J2000) before astrometric correction (Paper I)
DEC	float32	deg	Declination (J2000) before astrometric correction (Paper I)
Rad	int32	arcsec	Source extraction radius
Ann1	int32	arcsec	Inner radius of background extraction region
Ann2	int32	arcsec	Outer radius of background extraction region
REGAREA_s	float32	deg^2	Geometry area of source extraction region
Backscal_s	float32	deg^2	Source BACKSCAL
Backscal_b	float32	deg^2	Background BACKSCAL
FSclass	int32[1]		Class of 0.5-2 keV flux measurement. 0:model 5 (shape-fixed; faintest); 1:m2(double-powerlaw); 2:m6(0.4-2.2keV fit); 3:m0(APEC; stars)
FHclass	int32[1]		Class of 2.3-5 keV flux measurement. 0: model 5 (shape-fixed powerlaw; for faintest sources); 1: model 7 (powerlaw fitting in 2.3-6 keV)
Rate_d2_2d3	float32	counts/s	Net count rate in 0.2-2.3 keV
RateErr_d2_2d3	float32	counts/s	Net count rate error in 0.2-2.3 keV
Rate_d2_d5	float32	counts/s	Net count rate in 0.2-0.5 keV
RateErr_d2_d5	float32	counts/s	Net count rate error in 0.2-0.5 keV
Rate_d5_1	float32	counts/s	Net count rate in 0.5-1 keV
RateErr_d5_1	float32	counts/s	Net count rate error in 0.5-1 keV
Rate_1_2	float32	counts/s	Net count rate in 1-2 keV
RateErr_1_2	float32	counts/s	Net count rate error in 1-2 keV
Rate_2_4d5	float32	counts/s	Net count rate in 2-4.5 keV
RateErr_2_4d5	float32	counts/s	Net count rate error in 2-4.5 keV
Rate_2d3_5	float32	counts/s	Net count rate in 2.3-5 keV
RateErr_2d3_5	float32	counts/s	Net count rate error in 2.3-5 keV
Rate_5_8	float32	counts/s	Net count rate in 5-8 keV
RateErr_5_8	float32	counts/s	Net count rate error in 5-8 keV
BkgCts_d2_d6	float32	counts	Background counts in 0.2-0.6 keV
BkgCtsErr_d2_d6	float32	counts	Background counts error in 0.2-0.6 keV
BkgCts_d6_2d3	float32	counts	Background counts in 0.6-2.3 keV
BkgCtsErr_d6_2d3	float32	counts	Background counts error in 0.6-2.3 keV
BkgCts_2d3_5	float32	counts	Background counts in 2.3-5 keV
BkgCtsErr_2d3_5	float32	counts	Background counts error in 2.3-5 keV
BkgCts_5_8	float32	counts	Background counts in 5-8 keV
BkgCtsErr_5_8	float32	counts	Background counts error in 5-8 keV
PSFCor_d2_d5	float32		PSF-loss correction (ARF CORRPSF) averaged in 0.2-0.5 keV
PSFCor_d5_1	float32		PSF-loss correction (ARF CORRPSF) averaged in 0.5-1 keV
PSFCor_1_2	float32		PSF-loss correction (ARF CORRPSF) averaged in 1-2 keV
PSFCor_2d3_5	float32		PSF-loss correction (ARF CORRPSF) averaged in 2.3-5 keV
Nempty	int32		Number of empty channels between channel 20 and 900
FluxObsv_Med_s	float32	erg/cm^2/s	Observed flux in observed 0.5-2 keV, posterior median
FluxObsv_Lo1_s	float32	erg/cm^2/s	Observed flux in observed 0.5-2 keV, 1sigma lower limit
FluxObsv_Up1_s	float32	erg/cm^2/s	Observed flux in observed 0.5-2 keV, 1sigma upper limit
FluxObsv_Med_t	float32	erg/cm^2/s	Observed flux in observed 2.3-5 keV, posterior median
FluxObsv_Lo1_t	float32	erg/cm^2/s	Observed flux in observed 2.3-5 keV, 1sigma lower limit
FluxObsv_Up1_t	float32	erg/cm^2/s	Observed flux in observed 2.3-5 keV, 1sigma upper limit

Spectral fitting results with model 0: APEC

Broad-band fitting results using a single-temperature APEC model ("TBabs*apec" in Xspec), assuming the source is a star. Priors: z=0; log-uniform prior between 0.05 and 5 keV for kT; log-uniform prior between 4e19 and 4e20 cm^{-2} for Galactic N_H

Binary Table Caption for HDU1

Name	Type	Unit	Description
ID_SRC	int32		ID of the sources in the eFEDS main X-ray catalog (Paper I)
Redshift	float32		The redshift adopted for the spectral model
lognH_KL	float32	nats	log AGN column density, KL divergence
lognH_HLo	float32	cm^-2	log AGN column density, HDI lower limit
lognH_HUp	float32	cm^-2	log AGN column density, HDI upper limit
logkT_KL	float32	nats	log temperature, KL divergence
logkT_HLo	float32	keV	log temperature, HDI lower limit
logkT_HUp	float32	keV	log temperature, HDI upper limit
logAbundanc_KL	float32	nats	log abundance, KL divergence
logAbundanc_HLo	float32		log abundance, HDI lower limit
logAbundanc_HUp	float32		log abundance, HDI upper limit
lognH_BF	float32	cm^-2	log AGN column density, best-fit model
logkT_BF	float32	keV	log temperature, best-fit model
logAbundanc_BF	float32		log abundance, best-fit model
logApecNorm_BF	float32	cm^-5	log APEC normalization, best-fit model
FluxObsv_BF_s	float32	erg/cm^2/s	Observed flux in observed 0.5-2 keV, best-fit model
FluxObsv_Med_s	float32	erg/cm^2/s	Observed flux in observed 0.5-2 keV, posterior median
FluxObsv_Lo1_s	float32	erg/cm^2/s	Observed flux in observed 0.5-2 keV, 1sigma lower limit
FluxObsv_Up1_s	float32	erg/cm^2/s	Observed flux in observed 0.5-2 keV, 1sigma upper limit
FluxObsv_Lo2_s	float32	erg/cm^2/s	Observed flux in observed 0.5-2 keV, 2sigma lower limit
FluxObsv_Up2_s	float32	erg/cm^2/s	Observed flux in observed 0.5-2 keV, 2sigma upper limit
FluxObsv_BF_t	float32	erg/cm^2/s	Observed flux in observed 2.3-5 keV, best-fit model
FluxObsv_Med_t	float32	erg/cm^2/s	Observed flux in observed 2.3-5 keV, posterior median
FluxObsv_Lo1_t	float32	erg/cm^2/s	Observed flux in observed 2.3-5 keV, 1sigma lower limit
FluxObsv_Up1_t	float32	erg/cm^2/s	Observed flux in observed 2.3-5 keV, 1sigma upper limit
FluxObsv_Lo2_t	float32	erg/cm^2/s	Observed flux in observed 2.3-5 keV, 2sigma lower limit
FluxObsv_Up2_t	float32	erg/cm^2/s	Observed flux in observed 2.3-5 keV, 2sigma upper limit
lognH_Med	float32	cm^-2	log AGN column density, posterior median
lognH_Lo	float32	cm^-2	log AGN column density, percentile lower limit
lognH_Up	float32	cm^-2	log AGN column density, percentile upper limit
lognH_Mean	float32	cm^-2	log AGN column density, mean
lognH_Std	float32	cm^-2	log AGN column density, standard deviation
logkT_Med	float32	keV	log temperature, posterior median
logkT_Lo	float32	keV	log temperature, percentile lower limit
logkT_Up	float32	keV	log temperature, percentile upper limit
logkT_Mean	float32	keV	log temperature, mean
logkT_Std	float32	keV	log temperature, standard deviation
logAbundanc_Med	float32		log abundance, posterior median
logAbundanc_Lo	float32		log abundance, percentile lower limit
logAbundanc_Up	float32		log abundance, percentile upper limit
logAbundanc_Mean	float32		log abundance, mean
logAbundanc_Std	float32		log abundance, standard deviation
logApecNorm_Med	float32	cm^-5	log APEC normalization, posterior median
logApecNorm_Lo	float32	cm^-5	log APEC normalization, percentile lower limit
logApecNorm_Up	float32	cm^-5	log APEC normalization, percentile upper limit
logApecNorm_Mean	float32	cm^-5	log APEC normalization, mean
logApecNorm_Std	float32	cm^-5	log APEC normalization, standard deviation
logBkgNorm_Med	float32		log background normalization, posterior median
logBkgNorm_Lo	float32		log background normalization, percentile lower limit
logBkgNorm_Up	float32		log background normalization, percentile upper limit
logBkgNorm_Mean	float32		log background normalization, mean
logBkgNorm_Std	float32		log background normalization, standard deviation
chi25	float32		Chi^2 of the best-fit model against the rebinned data ( ≥25 cts/bin)
dof25	int32		DOF of the rebinned data, which has at least 25 counts per bin
logZ	float32[1]		log10 Bayesian evidence

Spectral fitting results with model 1: single-powerlaw

Broad-band fitting results using the ``single-powerlaw'' model ("TBabs*zTBabs*powerlaw" in Xspec). Priors: Gaussian(2.0,0.5) prior between -2 and 6 for Gamma; log-uniform prior between 4e19 and 4e24 cm^{-2} for AGN N_H

Binary Table Caption for HDU1

Name	Type	Unit	Description
ID_SRC	int32		ID of the sources in the eFEDS main X-ray catalog (Paper I)
Redshift	float32		The redshift adopted for the spectral model
Gamma_KL	float32	nats	power-law slope, KL divergence
Gamma_HLo	float32		power-law slope, HDI lower limit
Gamma_HUp	float32		power-law slope, HDI upper limit
lognH_KL	float32	nats	log AGN column density, KL divergence
lognH_HLo	float32	cm^-2	log AGN column density, HDI lower limit
lognH_HUp	float32	cm^-2	log AGN column density, HDI upper limit
Gamma_BF	float32		power-law slope, best-fit model
lognH_BF	float32	cm^-2	log AGN column density, best-fit model
logPowNorm_BF	float32	photons/keV/cm^2/s	log power-law normalization, best-fit model
FluxObsv_BF_s	float32	erg/cm^2/s	Observed flux in observed 0.5-2 keV, best-fit model
FluxObsv_Med_s	float32	erg/cm^2/s	Observed flux in observed 0.5-2 keV, posterior median
FluxObsv_Lo1_s	float32	erg/cm^2/s	Observed flux in observed 0.5-2 keV, 1sigma lower limit
FluxObsv_Up1_s	float32	erg/cm^2/s	Observed flux in observed 0.5-2 keV, 1sigma upper limit
FluxObsv_Lo2_s	float32	erg/cm^2/s	Observed flux in observed 0.5-2 keV, 2sigma lower limit
FluxObsv_Up2_s	float32	erg/cm^2/s	Observed flux in observed 0.5-2 keV, 2sigma upper limit
FluxObsv_BF_t	float32	erg/cm^2/s	Observed flux in observed 2.3-5 keV, best-fit model
FluxObsv_Med_t	float32	erg/cm^2/s	Observed flux in observed 2.3-5 keV, posterior median
FluxObsv_Lo1_t	float32	erg/cm^2/s	Observed flux in observed 2.3-5 keV, 1sigma lower limit
FluxObsv_Up1_t	float32	erg/cm^2/s	Observed flux in observed 2.3-5 keV, 1sigma upper limit
FluxObsv_Lo2_t	float32	erg/cm^2/s	Observed flux in observed 2.3-5 keV, 2sigma lower limit
FluxObsv_Up2_t	float32	erg/cm^2/s	Observed flux in observed 2.3-5 keV, 2sigma upper limit
FluxCorr_BF_s	float32	erg/cm^2/s	Absorption corrected flux in observed 0.5-2 keV, best-fit model
FluxCorr_Med_s	float32	erg/cm^2/s	Absorption corrected flux in observed 0.5-2 keV, posterior median
FluxCorr_Lo1_s	float32	erg/cm^2/s	Absorption corrected flux in observed 0.5-2 keV, 1sigma lower limit
FluxCorr_Up1_s	float32	erg/cm^2/s	Absorption corrected flux in observed 0.5-2 keV, 1sigma upper limit
FluxCorr_Lo2_s	float32	erg/cm^2/s	Absorption corrected flux in observed 0.5-2 keV, 2sigma lower limit
FluxCorr_Up2_s	float32	erg/cm^2/s	Absorption corrected flux in observed 0.5-2 keV, 2sigma upper limit
FluxCorr_BF_t	float32	erg/cm^2/s	Absorption corrected flux in observed 2.3-5 keV, best-fit model
FluxCorr_Med_t	float32	erg/cm^2/s	Absorption corrected flux in observed 2.3-5 keV, posterior median
FluxCorr_Lo1_t	float32	erg/cm^2/s	Absorption corrected flux in observed 2.3-5 keV, 1sigma lower limit
FluxCorr_Up1_t	float32	erg/cm^2/s	Absorption corrected flux in observed 2.3-5 keV, 1sigma upper limit
FluxCorr_Lo2_t	float32	erg/cm^2/s	Absorption corrected flux in observed 2.3-5 keV, 2sigma lower limit
FluxCorr_Up2_t	float32	erg/cm^2/s	Absorption corrected flux in observed 2.3-5 keV, 2sigma upper limit
FluxIntr_BF_s	float32	erg/cm^2/s	Absorption corrected flux in rest-frame 0.5-2 keV, best-fit model
FluxIntr_Med_s	float32	erg/cm^2/s	Absorption corrected flux in rest-frame 0.5-2 keV, posterior median
FluxIntr_Lo1_s	float32	erg/cm^2/s	Absorption corrected flux in rest-frame 0.5-2keV, 1sigma lower limit
FluxIntr_Up1_s	float32	erg/cm^2/s	Absorption corrected flux in rest-frame 0.5-2keV, 1sig upper limit
FluxIntr_Lo2_s	float32	erg/cm^2/s	Absorption corrected flux in rest-frame 0.5-2 keV, 2sig lower limit
FluxIntr_Up2_s	float32	erg/cm^2/s	Absorption corrected flux in rest-frame 0.5-2 keV, 2sig upper limit
FluxIntr_BF_h	float32	erg/cm^2/s	Absorption corrected flux in rest-frame 2-10 keV, best-fit model
FluxIntr_Med_h	float32	erg/cm^2/s	Absorption corrected flux in rest-frame 2-10 keV, posterior median
FluxIntr_Lo1_h	float32	erg/cm^2/s	Absorption corrected flux in rest-frame 2-10 keV, 1sigma lower limit
FluxIntr_Up1_h	float32	erg/cm^2/s	Absorption corrected flux in rest-frame 2-10 keV, 1sigma upper limit
FluxIntr_Lo2_h	float32	erg/cm^2/s	Absorption corrected flux in rest-frame 2-10 keV, 2sigma lower limit
FluxIntr_Up2_h	float32	erg/cm^2/s	Absorption corrected flux in rest-frame 2-10 keV, 2sigma upper limit
FluxIntr_BF_2keV	float32	erg/cm^2/s	Absorption corrected flux in rest-frame 1.999-2.001 keV, best-fit
FluxIntr_Med_2keV	float32	erg/cm^2/s	Absorption corrected flux in rest-frame 1.999-2.001 keV, median
FluxIntr_Lo1_2keV	float32	erg/cm^2/s	Absorption corrected flux in rest-f. 1.999-2.001keV, 1sig lowerlimit
FluxIntr_Up1_2keV	float32	erg/cm^2/s	Absorption corrected flux in rest-f. 1.999-2.001keV, 1sig upperlimit
FluxIntr_Lo2_2keV	float32	erg/cm^2/s	Absorption corrected flux in rest-f. 1.999-2.001keV, 2sig lowerlimit
FluxIntr_Up2_2keV	float32	erg/cm^2/s	Absorption corrected flux in rest-f. 1.999-2.001keV, 2sig upperlimit
LumiIntr_BF_s	float32	erg/s	Intrinsic luminosity in rest-frame 0.5-2 keV, best-fit model
LumiIntr_Med_s	float32	erg/s	Intrinsic luminosity in rest-frame 0.5-2 keV, posterior median
LumiIntr_Lo1_s	float32	erg/s	Intrinsic luminosity in rest-frame 0.5-2 keV, 1sigma lower limit
LumiIntr_Up1_s	float32	erg/s	Intrinsic luminosity in rest-frame 0.5-2 keV, 1sigma upper limit
LumiIntr_Lo2_s	float32	erg/s	Intrinsic luminosity in rest-frame 0.5-2 keV, 2sigma lower limit
LumiIntr_Up2_s	float32	erg/s	Intrinsic luminosity in rest-frame 0.5-2 keV, 2sigma upper limit
LumiIntr_BF_h	float32	erg/s	Intrinsic luminosity in rest-frame 2-10 keV, best-fit model
LumiIntr_Med_h	float32	erg/s	Intrinsic luminosity in rest-frame 2-10 keV, posterior median
LumiIntr_Lo1_h	float32	erg/s	Intrinsic luminosity in rest-frame 2-10 keV, 1sigma lower limit
LumiIntr_Up1_h	float32	erg/s	Intrinsic luminosity in rest-frame 2-10 keV, 1sigma upper limit
LumiIntr_Lo2_h	float32	erg/s	Intrinsic luminosity in rest-frame 2-10 keV, 2sigma lower limit
LumiIntr_Up2_h	float32	erg/s	Intrinsic luminosity in rest-frame 2-10 keV, 2sigma upper limit
LumiIntr_BF_2keV	float32	erg/s	Intrinsic luminosity in rest-frame 1.999-2.001 keV, best-fit model
LumiIntr_Med_2keV	float32	erg/s	Intrinsic luminosity in rest-frame 1.999-2.001 keV, posterior median
LumiIntr_Lo1_2keV	float32	erg/s	Intrinsic luminosity in rest-frame 1.999-2.001 keV, 1sig lower limit
LumiIntr_Up1_2keV	float32	erg/s	Intrinsic luminosity in rest-frame 1.999-2.001 keV, 1sig upper limit
LumiIntr_Lo2_2keV	float32	erg/s	Intrinsic luminosity in rest-frame 1.999-2.001 keV, 2sig lower limit
LumiIntr_Up2_2keV	float32	erg/s	Intrinsic luminosity in rest-frame 1.999-2.001 keV, 2sig upper limit
Gamma_Med	float32		power-law slope, posterior median
Gamma_Lo	float32		power-law slope, percentile lower limit
Gamma_Up	float32		power-law slope, percentile upper limit
Gamma_Mean	float32		power-law slope, mean
Gamma_Std	float32		power-law slope, standard deviation
lognH_Med	float32	cm^-2	log AGN column density, posterior median
lognH_Lo	float32	cm^-2	log AGN column density, percentile lower limit
lognH_Up	float32	cm^-2	log AGN column density, percentile upper limit
lognH_Mean	float32	cm^-2	log AGN column density, mean
lognH_Std	float32	cm^-2	log AGN column density, standard deviation
logPowNorm_Med	float32	photons/keV/cm^2/s	log power-law normalization, posterior median
logPowNorm_Lo	float32	photons/keV/cm^2/s	log power-law normalization, percentile lower limit
logPowNorm_Up	float32	photons/keV/cm^2/s	log power-law normalization, percentile upper limit
logPowNorm_Mean	float32	photons/keV/cm^2/s	log power-law normalization, mean
logPowNorm_Std	float32	photons/keV/cm^2/s	log power-law normalization, standard deviation
logBkgNorm_Med	float32		log background normalization, posterior median
logBkgNorm_Lo	float32		log background normalization, percentile lower limit
logBkgNorm_Up	float32		log background normalization, percentile upper limit
logBkgNorm_Mean	float32		log background normalization, mean
logBkgNorm_Std	float32		log background normalization, standard deviation
chi25	float32		Chi^2 of the best-fit model against the rebinned data ( ≥25 cts/bin)
dof25	int32		DOF of the rebinned data, which has at least 25 counts per bin
logZ	float32[1]		log10 Bayesian evidence
NHclass	int32[1]		Class of AGN NH measurement with model 1 (single-powerlaw). 1: uninformative; 2: unobscured; 3: mildly-measured; 4: well-measured

Spectral fitting results with model 2: double-powerlaw

Broad-band fitting results using the ``double-powerlaw'' model ("TBabs*zTBabs*(powerlaw+constant*spowerlaw)" in Xspec) for 16957 sources with at least 10 counts.

Priors: same priors as model 1 for Gamma and N_H; uniform prior between 0.5 and 5 for Delta_Gamma; log-uniform prior between 0.001 and 1 for the constant factor.

The "spowerlaw" is a power-law model whose slope equals the slope of the primary "powerlaw" plus Delta_Gamma.

Binary Table Caption for HDU1

Name	Type	Unit	Description
ID_SRC	int32		ID of the sources in the eFEDS main X-ray catalog (Paper I)
Redshift	float32		The redshift adopted for the spectral model
dGm_KL	float32	nats	Soft-powerlaw slope minus primary-powerlaw slope, KL divergence
dGm_HLo	float32		Soft-powerlaw slope minus primary-powerlaw slope, HDI lower limit
dGm_HUp	float32		Soft-powerlaw slope minus primary-powerlaw slope, HDI upper limit
Gamma_KL	float32	nats	power-law slope, KL divergence
Gamma_HLo	float32		power-law slope, HDI lower limit
Gamma_HUp	float32		power-law slope, HDI upper limit
lognH_KL	float32	nats	log AGN column density, KL divergence
lognH_HLo	float32	cm^-2	log AGN column density, HDI lower limit
lognH_HUp	float32	cm^-2	log AGN column density, HDI upper limit
logFrac_KL	float32	nats	Constant factor multiplied to the soft power-law, KL divergence
logFrac_HLo	float32		Constant factor multiplied to the soft power-law, HDI lower limit
logFrac_HUp	float32		Constant factor multiplied to the soft power-law, HDI upper limit
dGm_BF	float32		Soft-powerlaw slope minus primary-powerlaw slope, best-fit model
Gamma_BF	float32		power-law slope, best-fit model
lognH_BF	float32	cm^-2	log AGN column density, best-fit model
logPowNorm_BF	float32	photons/keV/cm^2/s	log power-law normalization, best-fit model
logFrac_BF	float32		Constant factor multiplied to the soft power-law, best-fit model
FluxObsv_BF_s	float32	erg/cm^2/s	Observed flux in observed 0.5-2 keV, best-fit model
FluxObsv_Med_s	float32	erg/cm^2/s	Observed flux in observed 0.5-2 keV, posterior median
FluxObsv_Lo1_s	float32	erg/cm^2/s	Observed flux in observed 0.5-2 keV, 1sigma lower limit
FluxObsv_Up1_s	float32	erg/cm^2/s	Observed flux in observed 0.5-2 keV, 1sigma upper limit
FluxObsv_Lo2_s	float32	erg/cm^2/s	Observed flux in observed 0.5-2 keV, 2sigma lower limit
FluxObsv_Up2_s	float32	erg/cm^2/s	Observed flux in observed 0.5-2 keV, 2sigma upper limit
FluxObsv_BF_t	float32	erg/cm^2/s	Observed flux in observed 2.3-5 keV, best-fit model
FluxObsv_Med_t	float32	erg/cm^2/s	Observed flux in observed 2.3-5 keV, posterior median
FluxObsv_Lo1_t	float32	erg/cm^2/s	Observed flux in observed 2.3-5 keV, 1sigma lower limit
FluxObsv_Up1_t	float32	erg/cm^2/s	Observed flux in observed 2.3-5 keV, 1sigma upper limit
FluxObsv_Lo2_t	float32	erg/cm^2/s	Observed flux in observed 2.3-5 keV, 2sigma lower limit
FluxObsv_Up2_t	float32	erg/cm^2/s	Observed flux in observed 2.3-5 keV, 2sigma upper limit
FluxCorr_BF_s	float32	erg/cm^2/s	Absorption corrected flux in observed 0.5-2 keV, best-fit model
FluxCorr_Med_s	float32	erg/cm^2/s	Absorption corrected flux in observed 0.5-2 keV, posterior median
FluxCorr_Lo1_s	float32	erg/cm^2/s	Absorption corrected flux in observed 0.5-2 keV, 1sigma lower limit
FluxCorr_Up1_s	float32	erg/cm^2/s	Absorption corrected flux in observed 0.5-2 keV, 1sigma upper limit
FluxCorr_Lo2_s	float32	erg/cm^2/s	Absorption corrected flux in observed 0.5-2 keV, 2sigma lower limit
FluxCorr_Up2_s	float32	erg/cm^2/s	Absorption corrected flux in observed 0.5-2 keV, 2sigma upper limit
FluxCorr_BF_t	float32	erg/cm^2/s	Absorption corrected flux in observed 2.3-5 keV, best-fit model
FluxCorr_Med_t	float32	erg/cm^2/s	Absorption corrected flux in observed 2.3-5 keV, posterior median
FluxCorr_Lo1_t	float32	erg/cm^2/s	Absorption corrected flux in observed 2.3-5 keV, 1sigma lower limit
FluxCorr_Up1_t	float32	erg/cm^2/s	Absorption corrected flux in observed 2.3-5 keV, 1sigma upper limit
FluxCorr_Lo2_t	float32	erg/cm^2/s	Absorption corrected flux in observed 2.3-5 keV, 2sigma lower limit
FluxCorr_Up2_t	float32	erg/cm^2/s	Absorption corrected flux in observed 2.3-5 keV, 2sigma upper limit
FluxIntr_BF_s	float32	erg/cm^2/s	Absorption corrected flux in rest-frame 0.5-2 keV, best-fit model
FluxIntr_Med_s	float32	erg/cm^2/s	Absorption corrected flux in rest-frame 0.5-2 keV, posterior median
FluxIntr_Lo1_s	float32	erg/cm^2/s	Absorption corrected flux in rest-frame 0.5-2keV, 1sigma lower limit
FluxIntr_Up1_s	float32	erg/cm^2/s	Absorption corrected flux in rest-frame 0.5-2keV, 1sig upper limit
FluxIntr_Lo2_s	float32	erg/cm^2/s	Absorption corrected flux in rest-frame 0.5-2 keV, 2sig lower limit
FluxIntr_Up2_s	float32	erg/cm^2/s	Absorption corrected flux in rest-frame 0.5-2 keV, 2sig upper limit
FluxIntr_BF_h	float32	erg/cm^2/s	Absorption corrected flux in rest-frame 2-10 keV, best-fit model
FluxIntr_Med_h	float32	erg/cm^2/s	Absorption corrected flux in rest-frame 2-10 keV, posterior median
FluxIntr_Lo1_h	float32	erg/cm^2/s	Absorption corrected flux in rest-frame 2-10 keV, 1sigma lower limit
FluxIntr_Up1_h	float32	erg/cm^2/s	Absorption corrected flux in rest-frame 2-10 keV, 1sigma upper limit
FluxIntr_Lo2_h	float32	erg/cm^2/s	Absorption corrected flux in rest-frame 2-10 keV, 2sigma lower limit
FluxIntr_Up2_h	float32	erg/cm^2/s	Absorption corrected flux in rest-frame 2-10 keV, 2sigma upper limit
FluxIntr_BF_2keV	float32	erg/cm^2/s	Absorption corrected flux in rest-frame 1.999-2.001 keV, best-fit
FluxIntr_Med_2keV	float32	erg/cm^2/s	Absorption corrected flux in rest-frame 1.999-2.001 keV, median
FluxIntr_Lo1_2keV	float32	erg/cm^2/s	Absorption corrected flux in rest-f. 1.999-2.001keV, 1sig lowerlimit
FluxIntr_Up1_2keV	float32	erg/cm^2/s	Absorption corrected flux in rest-f. 1.999-2.001keV, 1sig upperlimit
FluxIntr_Lo2_2keV	float32	erg/cm^2/s	Absorption corrected flux in rest-f. 1.999-2.001keV, 2sig lowerlimit
FluxIntr_Up2_2keV	float32	erg/cm^2/s	Absorption corrected flux in rest-f. 1.999-2.001keV, 2sig upperlimit
LumiIntr_BF_s	float32	erg/s	Intrinsic luminosity in rest-frame 0.5-2 keV, best-fit model
LumiIntr_Med_s	float32	erg/s	Intrinsic luminosity in rest-frame 0.5-2 keV, posterior median
LumiIntr_Lo1_s	float32	erg/s	Intrinsic luminosity in rest-frame 0.5-2 keV, 1sigma lower limit
LumiIntr_Up1_s	float32	erg/s	Intrinsic luminosity in rest-frame 0.5-2 keV, 1sigma upper limit
LumiIntr_Lo2_s	float32	erg/s	Intrinsic luminosity in rest-frame 0.5-2 keV, 2sigma lower limit
LumiIntr_Up2_s	float32	erg/s	Intrinsic luminosity in rest-frame 0.5-2 keV, 2sigma upper limit
LumiIntr_BF_h	float32	erg/s	Intrinsic luminosity in rest-frame 2-10 keV, best-fit model
LumiIntr_Med_h	float32	erg/s	Intrinsic luminosity in rest-frame 2-10 keV, posterior median
LumiIntr_Lo1_h	float32	erg/s	Intrinsic luminosity in rest-frame 2-10 keV, 1sigma lower limit
LumiIntr_Up1_h	float32	erg/s	Intrinsic luminosity in rest-frame 2-10 keV, 1sigma upper limit
LumiIntr_Lo2_h	float32	erg/s	Intrinsic luminosity in rest-frame 2-10 keV, 2sigma lower limit
LumiIntr_Up2_h	float32	erg/s	Intrinsic luminosity in rest-frame 2-10 keV, 2sigma upper limit
LumiIntr_BF_2keV	float32	erg/s	Intrinsic luminosity in rest-frame 1.999-2.001 keV, best-fit model
LumiIntr_Med_2keV	float32	erg/s	Intrinsic luminosity in rest-frame 1.999-2.001 keV, posterior median
LumiIntr_Lo1_2keV	float32	erg/s	Intrinsic luminosity in rest-frame 1.999-2.001 keV, 1sig lower limit
LumiIntr_Up1_2keV	float32	erg/s	Intrinsic luminosity in rest-frame 1.999-2.001 keV, 1sig upper limit
LumiIntr_Lo2_2keV	float32	erg/s	Intrinsic luminosity in rest-frame 1.999-2.001 keV, 2sig lower limit
LumiIntr_Up2_2keV	float32	erg/s	Intrinsic luminosity in rest-frame 1.999-2.001 keV, 2sig upper limit
dGm_Med	float32		Soft-powerlaw slope minus primary-powerlaw slope, posterior median
dGm_Lo	float32		Soft-powerlaw slope minus primary-powerlaw slope, 1sigma lower limit
dGm_Up	float32		Soft-powerlaw slope minus primary-powerlaw slope, 1sigma upper limit
dGm_Mean	float32		Soft-powerlaw slope minus primary-powerlaw slope, mean
dGm_Std	float32		Soft-powerlaw slope minus primary-powerlaw slope, standard devia.
Gamma_Med	float32		power-law slope, posterior median
Gamma_Lo	float32		power-law slope, percentile lower limit
Gamma_Up	float32		power-law slope, percentile upper limit
Gamma_Mean	float32		power-law slope, mean
Gamma_Std	float32		power-law slope, standard deviation
lognH_Med	float32	cm^-2	log AGN column density, posterior median
lognH_Lo	float32	cm^-2	log AGN column density, percentile lower limit
lognH_Up	float32	cm^-2	log AGN column density, percentile upper limit
lognH_Mean	float32	cm^-2	log AGN column density, mean
lognH_Std	float32	cm^-2	log AGN column density, standard deviation
logPowNorm_Med	float32	photons/keV/cm^2/s	log power-law normalization, posterior median
logPowNorm_Lo	float32	photons/keV/cm^2/s	log power-law normalization, percentile lower limit
logPowNorm_Up	float32	photons/keV/cm^2/s	log power-law normalization, percentile upper limit
logPowNorm_Mean	float32	photons/keV/cm^2/s	log power-law normalization, mean
logPowNorm_Std	float32	photons/keV/cm^2/s	log power-law normalization, standard deviation
logFrac_Med	float32		Constant factor multiplied to the soft power-law, posterior median
logFrac_Lo	float32		Constant factor multiplied to the soft power-law, 1sigma lower limit
logFrac_Up	float32		Constant factor multiplied to the soft power-law, 1sigma upper limit
logFrac_Mean	float32		Constant factor multiplied to the soft power-law, mean
logFrac_Std	float32		Constant factor multiplied to the soft power-law, standard devia.
logBkgNorm_Med	float32		log background normalization, posterior median
logBkgNorm_Lo	float32		log background normalization, percentile lower limit
logBkgNorm_Up	float32		log background normalization, percentile upper limit
logBkgNorm_Mean	float32		log background normalization, mean
logBkgNorm_Std	float32		log background normalization, standard deviation
chi25	float32		Chi^2 of the best-fit model against the rebinned data ( ≥25 cts/bin)
dof25	int32		DOF of the rebinned data, which has at least 25 counts per bin
logZ	float32[1]		log10 Bayesian evidence

Spectral fitting results with model 3: power-law plus blackbody

Broad-band fitting results using the powerlaw plus blackbody model ("TBabs*zTBabs*(powerlaw+zbbody)" in Xspec) for 16957 sources with at least 10 counts

Priors: same priors as model 1 for Gamma and N_H; log-uniform prior between 0.04 and 4 keV for kT

Binary Table Caption for HDU1

Name	Type	Unit	Description
ID_SRC	int32		ID of the sources in the eFEDS main X-ray catalog (Paper I)
Redshift	float32		The redshift adopted for the spectral model
Gamma_KL	float32	nats	power-law slope, KL divergence
Gamma_HLo	float32		power-law slope, HDI lower limit
Gamma_HUp	float32		power-law slope, HDI upper limit
lognH_KL	float32	nats	log AGN column density, KL divergence
lognH_HLo	float32	cm^-2	log AGN column density, HDI lower limit
lognH_HUp	float32	cm^-2	log AGN column density, HDI upper limit
logkT_KL	float32	nats	log temperature, KL divergence
logkT_HLo	float32	keV	log temperature, HDI lower limit
logkT_HUp	float32	keV	log temperature, HDI upper limit
Gamma_BF	float32		power-law slope, best-fit model
lognH_BF	float32	cm^-2	log AGN column density, best-fit model
logPowNorm_BF	float32	photons/keV/cm^2/s	log power-law normalization, best-fit model
logkT_BF	float32	keV	log temperature, best-fit model
logBBNorm_BF	float32	10^31 erg/s/pc^2	log blackbody normalization, best-fit model
Gamma_Med	float32		power-law slope, posterior median
Gamma_Lo	float32		power-law slope, percentile lower limit
Gamma_Up	float32		power-law slope, percentile upper limit
Gamma_Mean	float32		power-law slope, mean
Gamma_Std	float32		power-law slope, standard deviation
lognH_Med	float32	cm^-2	log AGN column density, posterior median
lognH_Lo	float32	cm^-2	log AGN column density, percentile lower limit
lognH_Up	float32	cm^-2	log AGN column density, percentile upper limit
lognH_Mean	float32	cm^-2	log AGN column density, mean
lognH_Std	float32	cm^-2	log AGN column density, standard deviation
logPowNorm_Med	float32	photons/keV/cm^2/s	log power-law normalization, posterior median
logPowNorm_Lo	float32	photons/keV/cm^2/s	log power-law normalization, percentile lower limit
logPowNorm_Up	float32	photons/keV/cm^2/s	log power-law normalization, percentile upper limit
logPowNorm_Mean	float32	photons/keV/cm^2/s	log power-law normalization, mean
logPowNorm_Std	float32	photons/keV/cm^2/s	log power-law normalization, standard deviation
logkT_Med	float32	keV	log temperature, posterior median
logkT_Lo	float32	keV	log temperature, percentile lower limit
logkT_Up	float32	keV	log temperature, percentile upper limit
logkT_Mean	float32	keV	log temperature, mean
logkT_Std	float32	keV	log temperature, standard deviation
logBBNorm_Med	float32	10^31 erg/s/pc^2	log blackbody normalization, posterior median
logBBNorm_Lo	float32	10^31 erg/s/pc^2	log blackbody normalization, percentile lower limit
logBBNorm_Up	float32	10^31 erg/s/pc^2	log blackbody normalization, percentile upper limit
logBBNorm_Mean	float32	10^31 erg/s/pc^2	log blackbody normalization, mean
logBBNorm_Std	float32	10^31 erg/s/pc^2	log blackbody normalization, standard deviation
logBkgNorm_Med	float32		log background normalization, posterior median
logBkgNorm_Lo	float32		log background normalization, percentile lower limit
logBkgNorm_Up	float32		log background normalization, percentile upper limit
logBkgNorm_Mean	float32		log background normalization, mean
logBkgNorm_Std	float32		log background normalization, standard deviation
chi25	float32		Chi^2 of the best-fit model against the rebinned data ( ≥25 cts/bin)
dof25	int32		DOF of the rebinned data, which has at least 25 counts per bin
logZ	float32[1]		log10 Bayesian evidence

Spectral fitting results with model 4: Gamma-fixed-powerlaw

Broad-band fitting results using the ``Gamma-fixed-powerlaw'' model. It is the same as model 1 but with fixed Gamma=2.0.

Binary Table Caption for HDU1

Name	Type	Unit	Description
ID_SRC	int32		ID of the sources in the eFEDS main X-ray catalog (Paper I)
Redshift	float32		The redshift adopted for the spectral model
lognH_KL	float32	nats	log AGN column density, KL divergence
lognH_HLo	float32	cm^-2	log AGN column density, HDI lower limit
lognH_HUp	float32	cm^-2	log AGN column density, HDI upper limit
lognH_BF	float32	cm^-2	log AGN column density, best-fit model
logPowNorm_BF	float32	photons/keV/cm^2/s	log power-law normalization, best-fit model
FluxObsv_BF_s	float32	erg/cm^2/s	Observed flux in observed 0.5-2 keV, best-fit model
FluxObsv_Med_s	float32	erg/cm^2/s	Observed flux in observed 0.5-2 keV, posterior median
FluxObsv_Lo1_s	float32	erg/cm^2/s	Observed flux in observed 0.5-2 keV, 1sigma lower limit
FluxObsv_Up1_s	float32	erg/cm^2/s	Observed flux in observed 0.5-2 keV, 1sigma upper limit
FluxObsv_Lo2_s	float32	erg/cm^2/s	Observed flux in observed 0.5-2 keV, 2sigma lower limit
FluxObsv_Up2_s	float32	erg/cm^2/s	Observed flux in observed 0.5-2 keV, 2sigma upper limit
FluxObsv_BF_t	float32	erg/cm^2/s	Observed flux in observed 2.3-5 keV, best-fit model
FluxObsv_Med_t	float32	erg/cm^2/s	Observed flux in observed 2.3-5 keV, posterior median
FluxObsv_Lo1_t	float32	erg/cm^2/s	Observed flux in observed 2.3-5 keV, 1sigma lower limit
FluxObsv_Up1_t	float32	erg/cm^2/s	Observed flux in observed 2.3-5 keV, 1sigma upper limit
FluxObsv_Lo2_t	float32	erg/cm^2/s	Observed flux in observed 2.3-5 keV, 2sigma lower limit
FluxObsv_Up2_t	float32	erg/cm^2/s	Observed flux in observed 2.3-5 keV, 2sigma upper limit
FluxCorr_BF_s	float32	erg/cm^2/s	Absorption corrected flux in observed 0.5-2 keV, best-fit model
FluxCorr_Med_s	float32	erg/cm^2/s	Absorption corrected flux in observed 0.5-2 keV, posterior median
FluxCorr_Lo1_s	float32	erg/cm^2/s	Absorption corrected flux in observed 0.5-2 keV, 1sigma lower limit
FluxCorr_Up1_s	float32	erg/cm^2/s	Absorption corrected flux in observed 0.5-2 keV, 1sigma upper limit
FluxCorr_Lo2_s	float32	erg/cm^2/s	Absorption corrected flux in observed 0.5-2 keV, 2sigma lower limit
FluxCorr_Up2_s	float32	erg/cm^2/s	Absorption corrected flux in observed 0.5-2 keV, 2sigma upper limit
FluxCorr_BF_t	float32	erg/cm^2/s	Absorption corrected flux in observed 2.3-5 keV, best-fit model
FluxCorr_Med_t	float32	erg/cm^2/s	Absorption corrected flux in observed 2.3-5 keV, posterior median
FluxCorr_Lo1_t	float32	erg/cm^2/s	Absorption corrected flux in observed 2.3-5 keV, 1sigma lower limit
FluxCorr_Up1_t	float32	erg/cm^2/s	Absorption corrected flux in observed 2.3-5 keV, 1sigma upper limit
FluxCorr_Lo2_t	float32	erg/cm^2/s	Absorption corrected flux in observed 2.3-5 keV, 2sigma lower limit
FluxCorr_Up2_t	float32	erg/cm^2/s	Absorption corrected flux in observed 2.3-5 keV, 2sigma upper limit
FluxIntr_BF_s	float32	erg/cm^2/s	Absorption corrected flux in rest-frame 0.5-2 keV, best-fit model
FluxIntr_Med_s	float32	erg/cm^2/s	Absorption corrected flux in rest-frame 0.5-2 keV, posterior median
FluxIntr_Lo1_s	float32	erg/cm^2/s	Absorption corrected flux in rest-frame 0.5-2keV, 1sigma lower limit
FluxIntr_Up1_s	float32	erg/cm^2/s	Absorption corrected flux in rest-frame 0.5-2keV, 1sig upper limit
FluxIntr_Lo2_s	float32	erg/cm^2/s	Absorption corrected flux in rest-frame 0.5-2 keV, 2sig lower limit
FluxIntr_Up2_s	float32	erg/cm^2/s	Absorption corrected flux in rest-frame 0.5-2 keV, 2sig upper limit
FluxIntr_BF_h	float32	erg/cm^2/s	Absorption corrected flux in rest-frame 2-10 keV, best-fit model
FluxIntr_Med_h	float32	erg/cm^2/s	Absorption corrected flux in rest-frame 2-10 keV, posterior median
FluxIntr_Lo1_h	float32	erg/cm^2/s	Absorption corrected flux in rest-frame 2-10 keV, 1sigma lower limit
FluxIntr_Up1_h	float32	erg/cm^2/s	Absorption corrected flux in rest-frame 2-10 keV, 1sigma upper limit
FluxIntr_Lo2_h	float32	erg/cm^2/s	Absorption corrected flux in rest-frame 2-10 keV, 2sigma lower limit
FluxIntr_Up2_h	float32	erg/cm^2/s	Absorption corrected flux in rest-frame 2-10 keV, 2sigma upper limit
FluxIntr_BF_2keV	float32	erg/cm^2/s	Absorption corrected flux in rest-frame 1.999-2.001 keV, best-fit
FluxIntr_Med_2keV	float32	erg/cm^2/s	Absorption corrected flux in rest-frame 1.999-2.001 keV, median
FluxIntr_Lo1_2keV	float32	erg/cm^2/s	Absorption corrected flux in rest-f. 1.999-2.001keV, 1sig lowerlimit
FluxIntr_Up1_2keV	float32	erg/cm^2/s	Absorption corrected flux in rest-f. 1.999-2.001keV, 1sig upperlimit
FluxIntr_Lo2_2keV	float32	erg/cm^2/s	Absorption corrected flux in rest-f. 1.999-2.001keV, 2sig lowerlimit
FluxIntr_Up2_2keV	float32	erg/cm^2/s	Absorption corrected flux in rest-f. 1.999-2.001keV, 2sig upperlimit
LumiIntr_BF_s	float32	erg/s	Intrinsic luminosity in rest-frame 0.5-2 keV, best-fit model
LumiIntr_Med_s	float32	erg/s	Intrinsic luminosity in rest-frame 0.5-2 keV, posterior median
LumiIntr_Lo1_s	float32	erg/s	Intrinsic luminosity in rest-frame 0.5-2 keV, 1sigma lower limit
LumiIntr_Up1_s	float32	erg/s	Intrinsic luminosity in rest-frame 0.5-2 keV, 1sigma upper limit
LumiIntr_Lo2_s	float32	erg/s	Intrinsic luminosity in rest-frame 0.5-2 keV, 2sigma lower limit
LumiIntr_Up2_s	float32	erg/s	Intrinsic luminosity in rest-frame 0.5-2 keV, 2sigma upper limit
LumiIntr_BF_h	float32	erg/s	Intrinsic luminosity in rest-frame 2-10 keV, best-fit model
LumiIntr_Med_h	float32	erg/s	Intrinsic luminosity in rest-frame 2-10 keV, posterior median
LumiIntr_Lo1_h	float32	erg/s	Intrinsic luminosity in rest-frame 2-10 keV, 1sigma lower limit
LumiIntr_Up1_h	float32	erg/s	Intrinsic luminosity in rest-frame 2-10 keV, 1sigma upper limit
LumiIntr_Lo2_h	float32	erg/s	Intrinsic luminosity in rest-frame 2-10 keV, 2sigma lower limit
LumiIntr_Up2_h	float32	erg/s	Intrinsic luminosity in rest-frame 2-10 keV, 2sigma upper limit
LumiIntr_BF_2keV	float32	erg/s	Intrinsic luminosity in rest-frame 1.999-2.001 keV, best-fit model
LumiIntr_Med_2keV	float32	erg/s	Intrinsic luminosity in rest-frame 1.999-2.001 keV, posterior median
LumiIntr_Lo1_2keV	float32	erg/s	Intrinsic luminosity in rest-frame 1.999-2.001 keV, 1sig lower limit
LumiIntr_Up1_2keV	float32	erg/s	Intrinsic luminosity in rest-frame 1.999-2.001 keV, 1sig upper limit
LumiIntr_Lo2_2keV	float32	erg/s	Intrinsic luminosity in rest-frame 1.999-2.001 keV, 2sig lower limit
LumiIntr_Up2_2keV	float32	erg/s	Intrinsic luminosity in rest-frame 1.999-2.001 keV, 2sig upper limit
lognH_Med	float32	cm^-2	log AGN column density, posterior median
lognH_Lo	float32	cm^-2	log AGN column density, percentile lower limit
lognH_Up	float32	cm^-2	log AGN column density, percentile upper limit
lognH_Mean	float32	cm^-2	log AGN column density, mean
lognH_Std	float32	cm^-2	log AGN column density, standard deviation
logPowNorm_Med	float32	photons/keV/cm^2/s	log power-law normalization, posterior median
logPowNorm_Lo	float32	photons/keV/cm^2/s	log power-law normalization, percentile lower limit
logPowNorm_Up	float32	photons/keV/cm^2/s	log power-law normalization, percentile upper limit
logPowNorm_Mean	float32	photons/keV/cm^2/s	log power-law normalization, mean
logPowNorm_Std	float32	photons/keV/cm^2/s	log power-law normalization, standard deviation
logBkgNorm_Med	float32		log background normalization, posterior median
logBkgNorm_Lo	float32		log background normalization, percentile lower limit
logBkgNorm_Up	float32		log background normalization, percentile upper limit
logBkgNorm_Mean	float32		log background normalization, mean
logBkgNorm_Std	float32		log background normalization, standard deviation
logZ	float32[1]		log10 Bayesian evidence

Spectral fitting results with model 5: shape-fixed-powerlaw

Detection-band (0.2-2.3 keV) fitting results using the ``shape-fixed-powerlaw'' model. It is the same as model 1 but with fixed N_H=0 and Gamma=2.0, leaving only the normalization parameters free.

Binary Table Caption for HDU1

Name	Type	Unit	Description
ID_SRC	int32		ID of the sources in the eFEDS main X-ray catalog (Paper I)
Redshift	float32		The redshift adopted for the spectral model
logPowNorm_BF	float32	photons/keV/cm^2/s	log power-law normalization, best-fit model
FluxObsv_BF_s	float32	erg/cm^2/s	Observed flux in observed 0.5-2 keV, best-fit model
FluxObsv_Med_s	float32	erg/cm^2/s	Observed flux in observed 0.5-2 keV, posterior median
FluxObsv_Lo1_s	float32	erg/cm^2/s	Observed flux in observed 0.5-2 keV, 1sigma lower limit
FluxObsv_Up1_s	float32	erg/cm^2/s	Observed flux in observed 0.5-2 keV, 1sigma upper limit
FluxObsv_Lo2_s	float32	erg/cm^2/s	Observed flux in observed 0.5-2 keV, 2sigma lower limit
FluxObsv_Up2_s	float32	erg/cm^2/s	Observed flux in observed 0.5-2 keV, 2sigma upper limit
FluxObsv_BF_t	float32	erg/cm^2/s	Observed flux in observed 2.3-5 keV, best-fit model
FluxObsv_Med_t	float32	erg/cm^2/s	Observed flux in observed 2.3-5 keV, posterior median
FluxObsv_Lo1_t	float32	erg/cm^2/s	Observed flux in observed 2.3-5 keV, 1sigma lower limit
FluxObsv_Up1_t	float32	erg/cm^2/s	Observed flux in observed 2.3-5 keV, 1sigma upper limit
FluxObsv_Lo2_t	float32	erg/cm^2/s	Observed flux in observed 2.3-5 keV, 2sigma lower limit
FluxObsv_Up2_t	float32	erg/cm^2/s	Observed flux in observed 2.3-5 keV, 2sigma upper limit
FluxCorr_BF_s	float32	erg/cm^2/s	Absorption corrected flux in observed 0.5-2 keV, best-fit model
FluxCorr_Med_s	float32	erg/cm^2/s	Absorption corrected flux in observed 0.5-2 keV, posterior median
FluxCorr_Lo1_s	float32	erg/cm^2/s	Absorption corrected flux in observed 0.5-2 keV, 1sigma lower limit
FluxCorr_Up1_s	float32	erg/cm^2/s	Absorption corrected flux in observed 0.5-2 keV, 1sigma upper limit
FluxCorr_Lo2_s	float32	erg/cm^2/s	Absorption corrected flux in observed 0.5-2 keV, 2sigma lower limit
FluxCorr_Up2_s	float32	erg/cm^2/s	Absorption corrected flux in observed 0.5-2 keV, 2sigma upper limit
FluxCorr_BF_t	float32	erg/cm^2/s	Absorption corrected flux in observed 2.3-5 keV, best-fit model
FluxCorr_Med_t	float32	erg/cm^2/s	Absorption corrected flux in observed 2.3-5 keV, posterior median
FluxCorr_Lo1_t	float32	erg/cm^2/s	Absorption corrected flux in observed 2.3-5 keV, 1sigma lower limit
FluxCorr_Up1_t	float32	erg/cm^2/s	Absorption corrected flux in observed 2.3-5 keV, 1sigma upper limit
FluxCorr_Lo2_t	float32	erg/cm^2/s	Absorption corrected flux in observed 2.3-5 keV, 2sigma lower limit
FluxCorr_Up2_t	float32	erg/cm^2/s	Absorption corrected flux in observed 2.3-5 keV, 2sigma upper limit
FluxIntr_BF_s	float32	erg/cm^2/s	Absorption corrected flux in rest-frame 0.5-2 keV, best-fit model
FluxIntr_Med_s	float32	erg/cm^2/s	Absorption corrected flux in rest-frame 0.5-2 keV, posterior median
FluxIntr_Lo1_s	float32	erg/cm^2/s	Absorption corrected flux in rest-frame 0.5-2keV, 1sigma lower limit
FluxIntr_Up1_s	float32	erg/cm^2/s	Absorption corrected flux in rest-frame 0.5-2keV, 1sig upper limit
FluxIntr_Lo2_s	float32	erg/cm^2/s	Absorption corrected flux in rest-frame 0.5-2 keV, 2sig lower limit
FluxIntr_Up2_s	float32	erg/cm^2/s	Absorption corrected flux in rest-frame 0.5-2 keV, 2sig upper limit
FluxIntr_BF_h	float32	erg/cm^2/s	Absorption corrected flux in rest-frame 2-10 keV, best-fit model
FluxIntr_Med_h	float32	erg/cm^2/s	Absorption corrected flux in rest-frame 2-10 keV, posterior median
FluxIntr_Lo1_h	float32	erg/cm^2/s	Absorption corrected flux in rest-frame 2-10 keV, 1sigma lower limit
FluxIntr_Up1_h	float32	erg/cm^2/s	Absorption corrected flux in rest-frame 2-10 keV, 1sigma upper limit
FluxIntr_Lo2_h	float32	erg/cm^2/s	Absorption corrected flux in rest-frame 2-10 keV, 2sigma lower limit
FluxIntr_Up2_h	float32	erg/cm^2/s	Absorption corrected flux in rest-frame 2-10 keV, 2sigma upper limit
FluxIntr_BF_2keV	float32	erg/cm^2/s	Absorption corrected flux in rest-frame 1.999-2.001 keV, best-fit
FluxIntr_Med_2keV	float32	erg/cm^2/s	Absorption corrected flux in rest-frame 1.999-2.001 keV, median
FluxIntr_Lo1_2keV	float32	erg/cm^2/s	Absorption corrected flux in rest-f. 1.999-2.001keV, 1sig lowerlimit
FluxIntr_Up1_2keV	float32	erg/cm^2/s	Absorption corrected flux in rest-f. 1.999-2.001keV, 1sig upperlimit
FluxIntr_Lo2_2keV	float32	erg/cm^2/s	Absorption corrected flux in rest-f. 1.999-2.001keV, 2sig lowerlimit
FluxIntr_Up2_2keV	float32	erg/cm^2/s	Absorption corrected flux in rest-f. 1.999-2.001keV, 2sig upperlimit
LumiIntr_BF_s	float32	erg/s	Intrinsic luminosity in rest-frame 0.5-2 keV, best-fit model
LumiIntr_Med_s	float32	erg/s	Intrinsic luminosity in rest-frame 0.5-2 keV, posterior median
LumiIntr_Lo1_s	float32	erg/s	Intrinsic luminosity in rest-frame 0.5-2 keV, 1sigma lower limit
LumiIntr_Up1_s	float32	erg/s	Intrinsic luminosity in rest-frame 0.5-2 keV, 1sigma upper limit
LumiIntr_Lo2_s	float32	erg/s	Intrinsic luminosity in rest-frame 0.5-2 keV, 2sigma lower limit
LumiIntr_Up2_s	float32	erg/s	Intrinsic luminosity in rest-frame 0.5-2 keV, 2sigma upper limit
LumiIntr_BF_h	float32	erg/s	Intrinsic luminosity in rest-frame 2-10 keV, best-fit model
LumiIntr_Med_h	float32	erg/s	Intrinsic luminosity in rest-frame 2-10 keV, posterior median
LumiIntr_Lo1_h	float32	erg/s	Intrinsic luminosity in rest-frame 2-10 keV, 1sigma lower limit
LumiIntr_Up1_h	float32	erg/s	Intrinsic luminosity in rest-frame 2-10 keV, 1sigma upper limit
LumiIntr_Lo2_h	float32	erg/s	Intrinsic luminosity in rest-frame 2-10 keV, 2sigma lower limit
LumiIntr_Up2_h	float32	erg/s	Intrinsic luminosity in rest-frame 2-10 keV, 2sigma upper limit
LumiIntr_BF_2keV	float32	erg/s	Intrinsic luminosity in rest-frame 1.999-2.001 keV, best-fit model
LumiIntr_Med_2keV	float32	erg/s	Intrinsic luminosity in rest-frame 1.999-2.001 keV, posterior median
LumiIntr_Lo1_2keV	float32	erg/s	Intrinsic luminosity in rest-frame 1.999-2.001 keV, 1sig lower limit
LumiIntr_Up1_2keV	float32	erg/s	Intrinsic luminosity in rest-frame 1.999-2.001 keV, 1sig upper limit
LumiIntr_Lo2_2keV	float32	erg/s	Intrinsic luminosity in rest-frame 1.999-2.001 keV, 2sig lower limit
LumiIntr_Up2_2keV	float32	erg/s	Intrinsic luminosity in rest-frame 1.999-2.001 keV, 2sig upper limit
logPowNorm_Med	float32	photons/keV/cm^2/s	log power-law normalization, posterior median
logPowNorm_Lo	float32	photons/keV/cm^2/s	log power-law normalization, percentile lower limit
logPowNorm_Up	float32	photons/keV/cm^2/s	log power-law normalization, percentile upper limit
logPowNorm_Mean	float32	photons/keV/cm^2/s	log power-law normalization, mean
logPowNorm_Std	float32	photons/keV/cm^2/s	log power-law normalization, standard deviation
logBkgNorm_Med	float32		log background normalization, posterior median
logBkgNorm_Lo	float32		log background normalization, percentile lower limit
logBkgNorm_Up	float32		log background normalization, percentile upper limit
logBkgNorm_Mean	float32		log background normalization, mean
logBkgNorm_Std	float32		log background normalization, standard deviation
logZ	float32[1]		log10 Bayesian evidence

Spectral fitting results with model 6: soft-band fitting

Soft-band (0.4-2.2 keV) fitting results using model 1: ``single-powerlaw''; only used to measure the 0.5-2 keV fluxes

Binary Table Caption for HDU1

Name	Type	Unit	Description
ID_SRC	int32		ID of the sources in the eFEDS main X-ray catalog (Paper I)
Redshift	float32		The redshift adopted for the spectral model
Gamma_KL	float32	nats	power-law slope, KL divergence
Gamma_HLo	float32		power-law slope, HDI lower limit
Gamma_HUp	float32		power-law slope, HDI upper limit
lognH_KL	float32	nats	log AGN column density, KL divergence
lognH_HLo	float32	cm^-2	log AGN column density, HDI lower limit
lognH_HUp	float32	cm^-2	log AGN column density, HDI upper limit
Gamma_BF	float32		power-law slope, best-fit model
lognH_BF	float32	cm^-2	log AGN column density, best-fit model
logPowNorm_BF	float32	photons/keV/cm^2/s	log power-law normalization, best-fit model
FluxObsv_BF_s	float32	erg/cm^2/s	Observed flux in observed 0.5-2 keV, best-fit model
FluxObsv_Med_s	float32	erg/cm^2/s	Observed flux in observed 0.5-2 keV, posterior median
FluxObsv_Lo1_s	float32	erg/cm^2/s	Observed flux in observed 0.5-2 keV, 1sigma lower limit
FluxObsv_Up1_s	float32	erg/cm^2/s	Observed flux in observed 0.5-2 keV, 1sigma upper limit
FluxObsv_Lo2_s	float32	erg/cm^2/s	Observed flux in observed 0.5-2 keV, 2sigma lower limit
FluxObsv_Up2_s	float32	erg/cm^2/s	Observed flux in observed 0.5-2 keV, 2sigma upper limit
Gamma_Med	float32		power-law slope, posterior median
Gamma_Lo	float32		power-law slope, percentile lower limit
Gamma_Up	float32		power-law slope, percentile upper limit
Gamma_Mean	float32		power-law slope, mean
Gamma_Std	float32		power-law slope, standard deviation
lognH_Med	float32	cm^-2	log AGN column density, posterior median
lognH_Lo	float32	cm^-2	log AGN column density, percentile lower limit
lognH_Up	float32	cm^-2	log AGN column density, percentile upper limit
lognH_Mean	float32	cm^-2	log AGN column density, mean
lognH_Std	float32	cm^-2	log AGN column density, standard deviation
logPowNorm_Med	float32	photons/keV/cm^2/s	log power-law normalization, posterior median
logPowNorm_Lo	float32	photons/keV/cm^2/s	log power-law normalization, percentile lower limit
logPowNorm_Up	float32	photons/keV/cm^2/s	log power-law normalization, percentile upper limit
logPowNorm_Mean	float32	photons/keV/cm^2/s	log power-law normalization, mean
logPowNorm_Std	float32	photons/keV/cm^2/s	log power-law normalization, standard deviation
logBkgNorm_Med	float32		log background normalization, posterior median
logBkgNorm_Lo	float32		log background normalization, percentile lower limit
logBkgNorm_Up	float32		log background normalization, percentile upper limit
logBkgNorm_Mean	float32		log background normalization, mean
logBkgNorm_Std	float32		log background normalization, standard deviation
logZ	float32[1]		log10 Bayesian evidence

Spectral fitting results with model 7: hard-band fitting

Hard-band (2.3-6 keV) fitting results using model 1: ``single-powerlaw'' for 2836 sources with at least 3 counts in the 2.3-5 keV band; only used to measure the 2.3-5 keV fluxes

Binary Table Caption for HDU1

Name	Type	Unit	Description
ID_SRC	int32		ID of the sources in the eFEDS main X-ray catalog (Paper I)
Redshift	float32		The redshift adopted for the spectral model
Gamma_KL	float32	nats	power-law slope, KL divergence
Gamma_HLo	float32		power-law slope, HDI lower limit
Gamma_HUp	float32		power-law slope, HDI upper limit
lognH_KL	float32	nats	log AGN column density, KL divergence
lognH_HLo	float32	cm^-2	log AGN column density, HDI lower limit
lognH_HUp	float32	cm^-2	log AGN column density, HDI upper limit
Gamma_BF	float32		power-law slope, best-fit model
lognH_BF	float32	cm^-2	log AGN column density, best-fit model
logPowNorm_BF	float32	photons/keV/cm^2/s	log power-law normalization, best-fit model
FluxObsv_BF_t	float32	erg/cm^2/s	Observed flux in observed 2.3-5 keV, best-fit model
FluxObsv_Med_t	float32	erg/cm^2/s	Observed flux in observed 2.3-5 keV, posterior median
FluxObsv_Lo1_t	float32	erg/cm^2/s	Observed flux in observed 2.3-5 keV, 1sigma lower limit
FluxObsv_Up1_t	float32	erg/cm^2/s	Observed flux in observed 2.3-5 keV, 1sigma upper limit
FluxObsv_Lo2_t	float32	erg/cm^2/s	Observed flux in observed 2.3-5 keV, 2sigma lower limit
FluxObsv_Up2_t	float32	erg/cm^2/s	Observed flux in observed 2.3-5 keV, 2sigma upper limit
FluxCorr_BF_t	float32	erg/cm^2/s	Absorption corrected flux in observed 2.3-5 keV, best-fit model
FluxCorr_Med_t	float32	erg/cm^2/s	Absorption corrected flux in observed 2.3-5 keV, posterior median
FluxCorr_Lo1_t	float32	erg/cm^2/s	Absorption corrected flux in observed 2.3-5 keV, 1sigma lower limit
FluxCorr_Up1_t	float32	erg/cm^2/s	Absorption corrected flux in observed 2.3-5 keV, 1sigma upper limit
FluxCorr_Lo2_t	float32	erg/cm^2/s	Absorption corrected flux in observed 2.3-5 keV, 2sigma lower limit
FluxCorr_Up2_t	float32	erg/cm^2/s	Absorption corrected flux in observed 2.3-5 keV, 2sigma upper limit
FluxIntr_BF_h	float32	erg/cm^2/s	Absorption corrected flux in rest-frame 2-10 keV, best-fit model
FluxIntr_Med_h	float32	erg/cm^2/s	Absorption corrected flux in rest-frame 2-10 keV, posterior median
FluxIntr_Lo1_h	float32	erg/cm^2/s	Absorption corrected flux in rest-frame 2-10 keV, 1sigma lower limit
FluxIntr_Up1_h	float32	erg/cm^2/s	Absorption corrected flux in rest-frame 2-10 keV, 1sigma upper limit
FluxIntr_Lo2_h	float32	erg/cm^2/s	Absorption corrected flux in rest-frame 2-10 keV, 2sigma lower limit
FluxIntr_Up2_h	float32	erg/cm^2/s	Absorption corrected flux in rest-frame 2-10 keV, 2sigma upper limit
LumiIntr_BF_h	float32	erg/s	Intrinsic luminosity in rest-frame 2-10 keV, best-fit model
LumiIntr_Med_h	float32	erg/s	Intrinsic luminosity in rest-frame 2-10 keV, posterior median
LumiIntr_Lo1_h	float32	erg/s	Intrinsic luminosity in rest-frame 2-10 keV, 1sigma lower limit
LumiIntr_Up1_h	float32	erg/s	Intrinsic luminosity in rest-frame 2-10 keV, 1sigma upper limit
LumiIntr_Lo2_h	float32	erg/s	Intrinsic luminosity in rest-frame 2-10 keV, 2sigma lower limit
LumiIntr_Up2_h	float32	erg/s	Intrinsic luminosity in rest-frame 2-10 keV, 2sigma upper limit
Gamma_Med	float32		power-law slope, posterior median
Gamma_Lo	float32		power-law slope, percentile lower limit
Gamma_Up	float32		power-law slope, percentile upper limit
Gamma_Mean	float32		power-law slope, mean
Gamma_Std	float32		power-law slope, standard deviation
lognH_Med	float32	cm^-2	log AGN column density, posterior median
lognH_Lo	float32	cm^-2	log AGN column density, percentile lower limit
lognH_Up	float32	cm^-2	log AGN column density, percentile upper limit
lognH_Mean	float32	cm^-2	log AGN column density, mean
lognH_Std	float32	cm^-2	log AGN column density, standard deviation
logPowNorm_Med	float32	photons/keV/cm^2/s	log power-law normalization, posterior median
logPowNorm_Lo	float32	photons/keV/cm^2/s	log power-law normalization, percentile lower limit
logPowNorm_Up	float32	photons/keV/cm^2/s	log power-law normalization, percentile upper limit
logPowNorm_Mean	float32	photons/keV/cm^2/s	log power-law normalization, mean
logPowNorm_Std	float32	photons/keV/cm^2/s	log power-law normalization, standard deviation
logBkgNorm_Med	float32		log background normalization, posterior median
logBkgNorm_Lo	float32		log background normalization, percentile lower limit
logBkgNorm_Up	float32		log background normalization, percentile upper limit
logBkgNorm_Mean	float32		log background normalization, mean
logBkgNorm_Std	float32		log background normalization, standard deviation
logZ	float32[1]		log10 Bayesian evidence

References

This section is the place to put references of interest.

Predehl et al. 2020. The eROSITA X-ray telescope on SRG

Paper I: Brunner et al. (submitted)

Paper II: Salvato et al. (submitted)

Acknowledgement

The eROSITA data model structure for catalogues was branched from the SDSS data model for value added catalogues.