Stellar mass-and-star formation rate (M_⊙ ⋅ yr⁻¹) plane in different redshift bins as labeled. The top row shows the whole sample analyzed in this work divided in star-forming (blue contours), green valley (green contours), and quiescent galaxies (red contours) based on the mass doubling time (see text for details). The middle row shows the distribution of late-type galaxies and the bottom row the one for early-type galaxies. In all panels, the solid line shows the mean of the posterior power-law fit to star-forming galaxies and the gray shaded regions indicates random samples of the posterior distribution. The dotted lines indicate the location ±1 dex around the main sequence.