Variation in M_*, sM_dust, and sSFR as a function of Hubble stage, from top to bottom panel, respectively. In each panel grey circles correspond to individual galaxies, black squares are the median values for each morphological bin. Error bars bracket the range between the 16^th and 84^th percentiles from the median. The curves, colour-coded with morphology (such as the data points in Figs. 2 and 3), are the fifth-order polynomial regressions to the median values (see Table B.1 for the polynomial regression parameters).