Fig. 5.
Unfolded FMPA (black) and FMPB (red) spectra of IGR J17503–2636 extracted using the entire exposure time available within the observation ID 90401333002. Right panel: results for the fit obtained with the model TBabs*(highecut*pegpwrlaw + Gaussian + Gaussian), while left panel corresponds to the case where the model TBabs*(highecut*pegpwrlaw*gabs + Gaussian) was used. In both cases, the residuals from the fits are shown in the bottom panels.
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