Table 4

X-ray spectral fit results from applying BXA to the extracted eROSITA and XRT spectra, with uncertainties enclosing 68% of the posterior for each parameter.

OBSID tbabs*blackbody tbabs*powerlaw


NH kT F0.2-2keV NH Γ F0.2-2keV
[ × 1020 cm−2 ] [eV] [ × 10−12 erg cm−2 s−1 ] [ × 1020cm−2] [ × 10−12 erg cm−2 s−1]
eRASS1
             
00013495001
             
00013495002
             
00013495003
             
00013495004
             
00013495005
             
00013495006

Notes. F0.2-2keV is the inferred observed (unabsorbed) flux under each model.

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