Ratios of the SFR_SED and the SFR_radio as a function of the SFR gradient over the last 300 Myr (∇SFR₃₀₀). Galaxies with ∇SFR₃₀₀ < 0 present a recent quenching, and galaxies with ∇SFR₃₀₀ > 0 present a recent starburst. Blue dots show instantaneous values of the SFR, and the orange, purple, and brown circles show an SFR_SED that was averaged for the last 100, 300, and 500 Myr, respectively. Black dots shows the mean trend and the dispersion of SFR ratio along the ∇SFR₃₀₀ inside a fixed bin size of 10°. The color-codes are the same as in Fig. 6.