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Fig. 9

image

M distribution of the sample, before (after) constraining AV on the top (bottom) panel. The best fitted SFHs are kept for each source. The overall distribution is affected very little by the constraining of the extinction in the fits, the shift toward lower masses is of the order of ~ 0.1 dex. The additional MS, starburst and quenching (see Sect. 4.2.4 for this last label) sub-groups, discriminated based on their position on the MSFR or SFRSED – SFRUV+IR diagrams, are discussed in Sect. 6.

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