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Fig. 8


Left panel: distribution of galaxies in the Log SFR – Log M plane, in which each bin (0.2 M in M and 0.2 M yr-1 in SFR) is colour-coded according to the weighted average value of the velocity dispersion σe in the bin. The white line represents the location of the MS of SFGs. Right panel: σe as a function of the distance from the MS, ΔMS, in six different bins of stellar mass, each 0.2 M wide. The different bins of stellar mass are indicated with different colours, as defined in the legend of the image, while the grey dotted vertical line represents the location of the MS. The error bars are obtained via bootstrapping.

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