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Fig. 1.


Distribution of the stellar masses for galaxies in the SIG sample according to their morphology (red solid line for early-type galaxies and blue dashed line for late-type galaxies in the top panel), colour (red solid line for red galaxies and blue dashed line for blue galaxies in the middle panel), and sSFR (red solid line for quenched galaxies and blue dashed line for star-forming galaxies in the lower panel). The shaded area in the figures corresponds to the selected stellar mass range for this study at 10.0  ≤  log(M)  ≤  11.4 M. The vertical black dotted line corresponds to the selected mass cut to distinguish between low-mass and high-mass galaxies at log(M)  =  10.6 M. The total number of galaxies at each side of the mass cut is indicated in the corresponding legend.

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