Fig. 3
a) NuSTAR-FPMA (dark blue), -FPMB (light blue), and Swift-XRT spectrum (red) of GRO J1008−57 in 2014 December after the second peak of its triple peaked outburst (epoch 3). The best-fit model is shown in black and the gray line shows its ratio to the spectral shape as predicted by our spectral evolution model (see Sect. 5 and Fig. 6). The data have been rebinned for display purposes. b) The residuals of the best-fit model.
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