Left panels: SFR–M_⋆ relation for galaxies in two regimes of LD, corresponding to the wings of the LD histograms shown in Fig. 9. Panels and lines are shown as Fig. 7. Cyan stars and the gold diamonds represent the median values of the SFR computed in 0.2 dex stellar mass bins, for the low- and high-LD regimes respectively. Error bars are computed as in Fig. 7. Right panels: histograms of the differences between the expected SFR computed using the main sequence fitting line at the stellar mass of any given galaxy in our sample and its actual SFR (ΔSFR). Median values of the distributions are shown with vertical dashed lines and colour coded as written in the legend.