Fig. C.4.
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Comparison of our best fit to all the data, with pBH = 0.1, with respect to different values from simulations on Mseed (Schauer et al. 2021; Kulkarni et al. 2021; Naoz & Barkana 2007), as well as the atomic cooling halo estimation at z = 20. The implications of the fit for the viability of posteriors in astrophysical terms are discussed in Sec. C.
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