Fig. 3

Local νIν spectra: impact of illumination computation (Newtonian or GR) and spin. Only one direction cosine is considered, cosi = 0.98 (almost face-on, i.e., close to the normal to the disk). The illumination is computed in general relativity (red) or in a Newtonian spacetime (black). The gray dotted spectrum is the blackbody function at the local temperature. The spin is 0 is the left column and 0.98 in the right column. The spectrum is computed at r = 2 M (upper row, right panel), r = 7 M (upper row left and middle panels) or r = 120 M (lower row).
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