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Fig. 6


sSFR distribution of the CANDELS sample in different z and stellar-mass bins. Each column shows a different redshift bin: (left), (central) and (right). Each row shows a different stellar-mass bin, with a width of 0.25 dex, from (top) to (bottom). Black thick continuous lines show the sSFR distribution and the yellow thin continuous lines are the best fitted models. Dotted lines are the different Gaussian components: quenched galaxies (red), MS galaxies (blue) and starburst galaxies (magenta). The and AIC values of each fit and the number of galaxies in each bin are shown in the top left of each panel. Grey areas show the sSFRs and stellar masses for which this sample is not complete (below the 3σ limit in sSFR or below the 90% completeness in stellar mass), or has statistics that are too low (N< 50).

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