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Fig. 7.

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MONK simulations of the Π and Ψ of the Comptonized+disk emission as a function of the energy in the 2–8 keV band for slab- and spreading layer-like configurations (blue and red respectively), along with a spreading layer case with the addition of the reflection component with Prefl = 10% and Ψrefl = 180° (green). The inclination of the system is 60°. The gray regions correspond to IXPE results at 90% confidence level obtained by applying polconst to the two best-fit models (Sect. 3.3). The polarization angle in MONK is measured from the projection of the rotation axis onto the sky plane.

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