Left panel: νL_ν (250 μm) normalised to the SFR as a function of stellar mass for z ≃ 0 GV galaxies (represented by filled circles). Quenching GV galaxies are in green and rejuvenating systems (transitioning from the RS to the GV) in orange. Median trends of the two galaxy samples are shown as solid lines, while shaded areas refer to the 16 − 84th percentile dispersions. Right panel: Distribution of the νL_ν (250 μm) normalised to the SFR for both quenching and rejuvenating GV galaxies (green and orange, respectively).