Normalized τ_dep (left), f_gas (mid-left), and T_dust (mid-right) by the scaling relation of τ_dep, scl(z, M_⋆, ΔMS) and f_gas, scl(z, M_⋆, ΔMS) from Tacconi et al. (2018) and of T_dust, scl(z, ΔMS) from Schreiber et al. (2018c) as well as the half-light radius R_e (right) at ALMA 1.13 mm as a function of ΔMS (first row) and M_⋆ (second row). Here, ΔMS is the distance to the SFMS (Schreiber et al. 2015), ΔMS = SFR/SFR_MS, at its own stellar mass and redshift for each sample. The blue dashed line and shaded area show the scaling relation and scatter. For each data point, the τ_dep, scl, f_gas, scl, and T_dust, scl are calculated at a fixed redshift, stellar mass, and ΔMS. Squares, stars, and shaded grey areas are the same as in Fig. 8.