Fig. 3
Cumulative stellar mass distribution of the star-forming galaxies in the UltraVISTA survey at z < 1 weighted by the SFR (dashed line) compared to that of the stellar masses of the LGRB hosts in our sample (dot-dashed line: whole sample; solid line: excluding the five host galaxies not complying with the completeness limits of the UltraVISTA survey).
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