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Fig. A.4

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Example of an unfolded spectrum taken with XMM-Newton EPIC-pn (orange), NuSTAR FPMA (red), and FPMB (blue) during the fourth NuSTAR orbit. Solid lines show the best-fit model with independent CFXMN and CFNuSTAR, and dotted lines account for best-fit model with tied CFs. First residual panel: Best-fit model with independent covering fractions. Second residual panel: Best-fit model with CFNuSTAR tied to CFXMN- Last residual panel: Best-fit model with CFXMN tied to CFNuSTAR- A strong soft excess in the NuSTAR data is visible at ~3 keV in comparison to the XMM-Newton data.

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