Fig. 7
a) 2007 Suzaku-spectrum of GRO J1008−57 (XISs:
orange, PIN: red, GSO: purple). Spectral channels are rebinned for display purposes.
b) A pure CUTOFFPL-model fitted to data above
5 keV, to compare with INTEGRAL-data (Coe et al. 2007), results in a poor description below that energy
(gray residuals). c) Adding a black body and a narrow iron line, and
taking absorption in the interstellar medium into account, improves the fit to
(1845 d.o.f.).
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