Fig. 12.
Upper panel: sMdust as a function of sSFR for LBGs derived from the SED fitting with CIGALE (full black triangles) and DGS galaxies (full red dots) overplotted with the distribution obtained from the likelihood analysis of chemical tracks described in Sect. 4 (empty symbols). Lower panel: sMdust as a function of age, colour coded as in the upper panel.
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