Fig. C.1.
Predictions of our model in two different scenarios, light-seed (“Pop III”) and heavy-seed (“Qc = 2.5”), for the mass function of black holes as a function of redshift. The model’s error bars are Poissonian. For comparison, also shown are the observational determinations of Shankar (2013) and Lauer et al. (2007) (at z = 0), and those of Merloni & Heinz (2008) and Schulze et al. (2015) (at z > 0).
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