Fig. 6.
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Effects of black hole spin on SED disk-fitting results. Top panel: SED of GB6 0805+614 with MCMC modeling results for a black hole with a = 0.998 and a = 0 overplotted in blue and orange, respectively. Bottom panel: Corner plot of posterior distributions for Ṁ,MBH, and λEdd for both spins (same color coding). Different (MBH,Ṁ) pairs produce identical accretion disk spectra.
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