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Fig. 6


Comparison between the artificially extended stellar mass cumulative distribution of the star-forming galaxies in the UltraVISTA survey at z < 1, weighted by the SFR, (dashed line) and that of the LGRB hosts in our sample (solid line: whole sample; dotted lines: excluding three GRBs as explained in the text). Illustrated here is the slope of unity case for the SFR–M relation (see text for details).

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