Currently observed sSFR of MaNGA galaxies compared to their M_* (bottom left). The black contours enclose 95%, 65% and 35% of the sample respectively. The green line is the median sSFR within 0.25 dex wide M_* bins. In the top and right panels, the distributions in M_* and sSFR, respectively, are shown as histograms, with the three morphological bins shown in lines of the corresponding colour.