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Table 4

X-ray spectral modelling of intensity-resolved eROSITA spectra.

Obs. Component Parameter Value (Flare) Value (Flare removed) Units
1 TBabs N 0.0618 (fixed) 1022 cm−2
           
TBvarabs N 1.3 ± 0.4 2.7 ± 0.6 1022 cm−2
Powerlaw Γ 0.98
Constant factor 1.0 (fixed) 0.24 ± 0.04
Fx 4.1 ± 1.0 0.9 ± 0.2 10−12 erg cm−2 s−1
Lx 1.2 0.2 1036 erg s−1
3 TBabs N 0.0618 (fixed) 1022 cm−2
           
TBvarabs N 1.4 ± 0.5 3.5 ± 0.7 1022 cm−2
Powerlaw Γ 0.92
Constant factor 1.0 (fixed) 0.56 ± 0.10
Fx 4.4 ± 1.0 2.3 ± 0.5 10−12 erg cm−2 s−1
Lx 1.4 0.8 1036 erg s−1

Notes. Results from a simultaneous fit of an absorbed power-law model (TBabs*TBvarabs*powerlaw) to the eROSITA intensity-resolved spectra. Fluxes and luminosities are integrated over the 0.2–10.0 keV energy band. Lx are corrected for absorption assuming a distance of 50 kpc.

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