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Fig. 3.


Infrared star formation rate as a function of redshift, for galaxies from the main (red dots) and supplementary (gray dots) catalogs respectively. The SFR has been computed from the IR luminosity following Eq. (10). The detection limits at 4.8σ (solid black line) and 3.5σ (dashed black line) have also been computed from the IR library of Schreiber et al. (2018b), with a dust temperature evolving with redshift taking into account the average value of the rms at 0.182 mJy.

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