Fig. 6
EGB spectrum. The blue and red shaded regions correspond to AGN winds and starburst galaxies predicted by our SAM, respectively. The purple shaded region corresponds to the contribution to the EGB from AGN winds estimated by Wang & Loeb (2016a). The cyan and gold lines indicate the estimate for quiescent and starburst galaxies, respectively, predicted by the Makiya et al. (2011) SAM. The green shaded region shows the contribution to the EGB from blazars as estimated by Ajello et al. (2015). The data points are as in Fig. 4.
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