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Fig. 4

image

SFRM plane with the best linear fits to all SF galaxies at different redshifts: (left), (center) and (right). The slope of each sequence is reported on the top-left of each panel. In the background there are all the SF galaxies in our sample above the stellar mass completeness, divided into SFRM bins of 0.1 × 0.1 dex. Each bin is colour-coded depending on the number of galaxies inside each bin, from green to yellow in a linear scale. The vertical black dotted lines are the 90% completeness limit in stellar mass in each redshift bin; galaxies below this limit are plotted as grey points and are not included in the fit. The horizontal dotted black lines are the 3σ detection limit in SFR in each redshift bin.

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