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Fig. 8.

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Positions of the n = 0 (left panels) and n = 1 (right panels) peaks, observed at 345 GHz and i = 163°, for all the possible emission configurations computed including the real value of the synchrotron pitch angle, θB, for a vertical magnetic field in the case of a Schwarzschild black hole (green), a RZ black hole with a1|ϵ = 0 = 0.1 (pink), and a RZ black hole with ϵ |a1 = 0 = 0.1 (violet). Each row corresponds to a different velocity: Keplerian, radial or mixed. Critical curves are represented as dashed lines.

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