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Fig. 1


Distribution of galaxies in SALL sample in the Log SFR – Log M plane. Top panels: SFR distribution of galaxies in three different stellar mass bins. The red solid line is the result of the gaussian fit to the right-side of the SF peak. Bottom panel: Log SFR – Log M plane colour-coded as a function of the number of galaxies in each bin. The contours encircle bins that host a number of galaxies from 50 to 1250, with step of 250. The MS of SFGs is indicated by the thick solid line, while the error bars mark the 1σ scatter.

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