Evolution of the sSFR over cosmic time for the galaxies in the MaNGA sample. In each panel the M_* and sSFR of the galaxies measured at different LBT are shown. The colour of the data points corresponds to the currently observed morphology of the galaxies. The black contours enclose 95%, 65% and 35% of the sample, respectively. The cyan and violet dots and lines show the median sSFR within 0.5 dex wide M_* bins, selecting galaxies above and below 6 Å in EW_Hα, respectively. The error bars for the dots show the 25th and 75th percentile of the distribution within each M_* bin.