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Fig. 6.
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10–50 keV luminosity as a function of BH mass. The grey circles show the model predictions, estimated using KYNSED for various combinations of height, a*, ṁEdd, and Rtr. The red squares show the observed values for QJ 0158, HE 0435, SDSS 0924, SDSS 1004, HE 1104, and Q 2237, from Chen et al. (2012) (see text for details).
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