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Fig. 7


SFRM plane with the best ODR fits for the three galaxy modes: quenched galaxies (red line), MS galaxies (blue line) and SB galaxies (magenta line). The slope of each sequence is reported in the top-left of each panel. Squared symbols are the Gaussian peak positions of the three components in each stellar mass bin with the associated error in the position. In the background there are all galaxies in our sample 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. The horizontal dotted black lines are the 3σ detection limit in SFR in each redshift bin.

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