From top to bottom (first four panels): , sSFR and as a function of Hubble stages (T). In each panel orange circles are individual galaxies, red diamonds are the mean values for each morphological bin, while blue squares are the median values. Error bars bracket the range between the 16th and 84th percentiles from the median. The thick green curves are fifth-order polynomial regressions to the median values (see Table D.1 for the polynomial regression parameters). In each of these panels “+” and “X” symbols indicate strong radio jet galaxies and AGNs, respectively. The last panel shows the variation in M_star, , M_HI, and SFR (red, orange, magenta, and cyan lines respectively) with morphology as being fitted with a fifth-order polynomial regression through the median values (see Table D.1). M_star, , M_HI, and SFR have been normalized to the maximum value obtained from each polynomial regression by: 3.9 × 10¹⁰ M_⊙, 1.2 × 10⁷ M_⊙, 2.6 × 10⁹ M_⊙ and 1.08 M_⊙ yr⁻¹, respectively.