Fig. A.1.
Measurements of the SFRD using galaxy surveys (Madau & Dickinson 2014). The solid black line shows the SFRD as measured by the CIB linear model of Maniyar et al. (2018). The solid blue line shows the corresponding constraints when the SFRD values from the galaxies are not considered as priors while performing the fit of the CIB halo model. The dotted black and red lines show the 1σ regions.
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