Fig. 11.

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Black hole mass as a function of the semi-major axis of the hotspot’s orbit. The orbital period is fixed to the observed one, Ps = 75.4 days. Peng et al. (2006) estimates of the black hole mass imply that the emission region of the disk at the origin of the periodic signal is located at around 120rg from the central black hole. The vertical blue line indicates the ISCO for a Schwarzschild black hole.
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