Fig. 5.
Measurements of the infrared SFRD using galaxies (Madau & Dickinson 2014). The solid black (blue) line shows the SFRD as constrained by the linear (halo) model with the dotted black (dotted blue) lines showing the 1σ regions around it. We also show the SFRD value determined by Khusanova et al. completely independently using the data from the ALMA ALPINE large program (priv. comm.).
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