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Fig. 2.

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Influence of relativistic effects on the PA and the emission angle. The rotation of the PA (a sum of the GR and SR effects) χtot (upper panels) and the emission angle ζ′ (lower panels) computed at r = rISCO (given in the upper left corner of each panel) for spins a = 0.2 (left panels), 0.5 (middle panels), and 0.8 (right panels) at three inclinations i = 30° (red), 60° (green), and 80° (blue lines). The results using ARTPOL code are shown with the solid lines, while the results from the ray-tracing in Kerr metric are presented with the dashed lines. The difference between the two values is shown under each panel.

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