Fig. B.1
KERRBB disk bolometric luminosity as a function of the viewing angle of the disk, fitted bythe best function (Eq. (B.1), blue lines) and the polynomial function (Eq. (B.3), red lines) for different spin values. Dots represent the KERRBB results with Ṁ = 1018 g/s. By increasing the spin, the differences between the two functions grow.
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