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Fig. C.6.

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Widths of the n = 0 (left panels) and n = 1 (right panels) images for all the possible emission configurations 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). The velocity of the disc is taken to be Keplerian for the upper panels, radial for the central panels, and mixed for the lower panels.

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