Fig. 2
a) The Suzaku-XIS (0: blue; 1: yellow; 3: green), -PIN (red), and -GSO (purple) spectra of the 2014 January observation of GRO J1008−57 (epoch 2) together with the best-fit model (black). b–d) The residuals to the best-fit model (b: XIS0, PIN, and GSO; c: XIS1; d: XIS3) showing the ignored energy bins due to calibration uncertainties (gray). The residuals of XIS1 (c) are shown without taking the photon index shift, ΔΓ, into account.
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