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Fig. 1


Cumulative distribution of the K luminosity (LK) of the star-forming galaxies in the UltraVISTA survey at z < 1 (dotted line) weighted by the SFR (dashed line) compared to that of the LGRB hosts in our sample (solid line: without the three LGRB host galaxies not complying with the UltraVISTA redshift and K-band magnitude cuts; dot-dashed line: whole sample).

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