Fig. 10.

Fraction of star-forming galaxies in different bins of LD, computed with the sSFR (left panels) and rest-frame colour (right panels). Three redshift bins from z = 0.1 up to z = 0.5 are represented, and the redshift increases from top to bottom panels as indicated in each panel. A sigma-clipping has been performed on the parent LD distributions to remove outliers and bins with a non-statistically representative number of objects. Panels and symbols are shown as in Fig. 6.
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