Fig. 4.
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Polarization fraction (Π), summed between 2 and 8 keV, as a function of the inclination of the source, assuming different wedge opening angles. In both panels, the coronal temperature is set to kTe = 60 keV and Rdisk = 25RG. The left panel corresponds to the a = 0 and Rcorona = 6RG scenario, while the right panel corresponds to a = 0.998 and Rcorona = 1.24RG scenario. As the opening angle increases, Π decreases due to the increasing degree of symmetry of the system.
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