Evolution of massive galaxy properties from their low-z values out to z ∼ 1. Relationships for molecular gas to stellar mass ratio (M_H2/M_*), specific SFR, SFR efficiency (SFR/M_H2), and metallicity (log(O/H)+12) are from the A³COSMOS scaling relations for main-sequence galaxies derived by Liu et al. (2019), adopting the Schreiber et al. (2015) main-sequence. Solid lines show the relations at log(M_*/M_⊙) = 10.2 and dotted lines show the relations for galaxies with log(M_*/M_⊙) = 11.5. Unlike (Leslie et al. 2018a, L18), who found that F increases with redshift and the τ_B remains constant to z ∼ 0.7, we find that both these dust parameters evolve together increasing by a factor of ∼1.7 () and ∼1.8 (F) from low-z galaxies in GAMA and SDSS to intermediate-redshift galaxies in COSMOS.