Fig. 7.

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Best fit of the IXPE and NuSTAR spectra. Left panel: IXPE and NuSTAR deconvolved spectra with best-fitting model (see Table 3) and residuals. The model includes diskbb (dashed dotted line), comptb (dashed line), and relxillns (dotted line). Right panel: IXPE Q and U Stokes spectra with the best-fitting model, assuming either comptb (solid lines) or diskbb (dashed lines) as the only polarized component, and the corresponding residuals. Data from different detectors were combined (with setplot group) for plotting purposes.
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