Median sSFR profiles in the last 30 Myr obtained from the SFHs (dots connected with thick solid lines). The sSFR values below ∼10⁻¹² yr⁻¹ are very uncertain and can be considered as upper limits. The left column is for CLEs, the central column is for RQEs, and the right column is for BSFs. Each row is a stellar-mass bin, which increases from the bottom to the top. The shaded regions in the left panels correspond to the 16th and 84th percentiles. Given the relatively low numbers of RQE and BSF galaxies, we show the individual profiles as thin lines. The number of galaxies of each type in a given mass bin is shown in each panel. The horizontal error bar is the typical PSF, which represents the minimum radial resolution of the IFU.