Fig. 6.
Comparison between the full GR simulated spectrum (stars) of the unperturbed, pre-RWI disc with the cases of a standard disc model with either a Minkowski ray-tracing (diskbb equivalent) or a general relativistic Kerr ray-tracing for a case where a = 0.98 with an inclination angle of 70°. The corner plot is the same plot in log-log.
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