Ratio of the SFR and SFR_radio as a function of the SFR gradient over the last 300 Myr (∇SFR₃₀₀). In perfect scenarios in which the two indicators give the same value, we expect a uniform distribution centered at 1 (but 0 in log) over the SFRs ratios along the ∇SFR₃₀₀. The shaded red region shows galaxies with negative values of the ∇SFR₃₀₀ (i.e., quenched) and an SFR ratio lower than 0.1, and the shaded region shows galaxies with positive values of the ∇SFR₃₀₀ (i.e., starbursting) and an SFR ratio higher than 0.1. The dots are color-coded according to the instantaneous SFR derived from the SED fitting procedure. The mean error bars are shown as black crosses for galaxies inside regions (A) and (B).