Atomic hydrogen mass (left), (middle) and dust mass (right) to stellar mass ratio as a function of the distance to the MS (sSFR/sSFR_MS). Symbols are the same as Fig. 16. Symbols are colored by gas fraction, with gray symbols used for sources with unknown gas fraction. The vertical line divides the galaxies with low and normal sSFR (PAS, InPAS and MS to the left), and galaxies with high sSFR (InSB and SB to the right). The black cross shows the typical error.