Fig. A.1.
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Star formation rate against stellar mass for GRB hosts and star-forming galaxies of the 3D-HST survey. Two redshift bins are considered, at 1 < z < 2 (top panel) and 2 < z < 3.1 (bottom panel). The star-forming galaxies selected in the analysis combining SFRUV+IR and SFRUV,corr values are plotted in background as a 2D gray histogram. The blue and dark blue curves are the main sequence relations derived by Whitaker et al. (2014) at 1 < z < 2.5.
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