Fig. 9
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Results of the phase-averaged spectral fitting. Top: we show the eROSITA spectra of detectors 2, 3, 4, and 6 simultaneously fit by the model of Table 6 and a fixed power-law index of Γ = 1.98. Bottom: simultaneous fit of eROSITA, XMM-Newton, and NuSTAR (dark gray, magenta, and blue data points, respectively). The best-fit parameters are listed in Table 6.
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