Overview of the properties of our sample as a function of the Hubble stage parameter (HT). From top to bottom: histogram of the number of galaxies in each bin (ΔT = 1); the distribution of the masses of different components, molecular (M_H2) and atomic (M_HI) gas, the dust (M_dust) and stars (M_⋆), respectively; SFR, molecular-to-total gas fraction, and metallicity. Data are represented as gray points, the mean value in each bin of HT is a red circle. In each panel, we indicate the number of galaxies with measurements (and upper limits) for each quantity. This figure is similar to Fig. 1 by C20.