Table 1

Catalogs presented in this work.

Index Table name and number Table description Sample selection criteria or Xspec model and prior
1 AGN The eFEDS AGN catalog Sources from the main X-ray catalog with extent like-lihood = 0, counterpart quality ⩾2, and classified as “Likely galactic” or “Secure galacitc”.
2 Spec Model-independent spectral properties and observed source fluxes All sources in the main X-ray catalog
3 m0:apec0 Broad-band fitting (0.2–8 keV) using a single-temperature APEC model; only useful for stars TBabs*apec z = 0; log-uniform prior between 0.05 and 5 keV for kT; log-uniform prior between 4 × 1019 and 4 × 1020 cm–2 for Galactic NH
4 m1:pow Broad-band fitting (0.2–8 keV) results using the single-powerlaw model TBabs*zTBabs*powerlaw Gaussian(2.0,0.5) prior between -2 and 6 for Γ; log-uniform prior between 4 × 1019 and 4 × 1024 cm–2 for AGN NH
5 m2:powpow Broad-band fitting (0.2–8 keV) results using the double-powerlaw model TBabs*zTBabs*(powerlaw+constant*spowerlaw)14 same priors as model 1 for Γ and NH; uniform prior between 0.5 and 5 for ∆Γ; log-uniform prior between 0.001 and 1 for the constant factor
6 m3:powbb Broad-band fitting (0.2–8 keV) results using the powerlaw + blackbody model TBabs*zTBabs*(powerlaw+zbbody) same priors as model 1 for Γ and NH, log-uniform prior between 0.04 and 4 keV for kT
7 m4:pow2d0 Broad-band fitting (0.2–8 keV) results using the Γ-fixed-powerlaw model Same as model 1 but fixing Γ = 2.0
8 m5:powfix Detection-band (0.2–2.3 keV) fitting results using the shape-fixed-powerlaw model Same as model 1 but fixing NH = 0 and Γ = 2.0
9 m6:soft Soft-band (0.4–2.2 keV) fitting results using the single-powerlaw model; only used to measure the 0.5–2keV fluxes. Same as model 1 but in a soft, narrow band
10 m7:hard Hard-band (2.3–6 keV) fitting results using the single-powerlaw model; only used to measure the 2.3–5 keV fluxes. Same as model 1 but in a hard, narrow band

Notes. The index is the extension number in the merged FITS-format file. The spectral fitting result tables are named so as to include the model index i in terms of mi before the colon.

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