Top row: τ_dep (first column), f_gas (second column), and T_dust (third column) as a function of Σ_SFR. Only galaxies with a Herschel counterpart with the most reliable size measurements in Gómez-Guijarro et al. (2022) are shown (corresponding to a detection S/N_peak ≥ 6.5). SBs in the MS are in red. Galaxies identified as AGN are highlighted with diamonds. All galaxies are color coded according to their ΔMS. Bottom row: deviations of τ_dep (first column), f_gas (second column), and T_dust (third column) compared to the gas scaling relations of normal MS SFGs (ΔMS = 1) in relation with the deviations of the dust continuum areas compared to the structural scaling relation of normal SFGs at a fixed stellar mass and redshift. The gas scaling relations for τ_dep(z, M_*, ΔMS) and f_gas(z, M_*, ΔMS) are from Tacconi et al. (2018), and for T_dust(z, ΔMS) from Schreiber et al. (2018), where ΔMS = 1. In the case of the structural scaling relation, we compared the dust continuum areas with the typical areas of star-forming stellar disks measured at optical wavelengths for late-type galaxies from van der Wel et al. (2014), at a fixed stellar mass and redshift. The stack of the 23/69 galaxies that were classified as SBs in the MS originally in Fig. 3 is shown as an empty red square (where the total number of galaxies accounts only for galaxies with a Herschel counterpart). Similarly, the stack of the remaining galaxies that were not labeled as SBs in the MS in Fig. 3 are shown as an empty black square.