Fig. A.1.

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Left: Accretion rate (log ṁ/ṁEdd) as a function of the Eddington ratio (log λEdd). The solid line show the identity line. The bottom panel shows the difference between log ṁ/ṁEdd and the identity line. Middle: Same but replacing the x-axis with the sum of log λEdd and a polynomial function of the inclination angle to account for the anisotropy in the emission (see text for more details). The colour maps corresponds to μ = cos i. Bottom right: Distribution of the differences between the y-axis and the x-axis in the left and middle panels (blue and red histograms, respectively)
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