Fig. B.1.
Inverse-Compton protogalaxy X-ray luminosity evolution over redshift, as calculated using the approach detailed in this paper with ℛSN ≈ 1 yr−1 (semi-analytical Monte-Carlo simulation) compared to the earlier study, Schober et al. (2015) (dashed grey line), which adopts an analytical model. Our results are consistent with those obtained by Schober et al. (2015).
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