sM_Dust plotted against sSFR for the ALPINE galaxies assuming a Chabrier IMF (left panel) and THIMF (right panel). The circles indicate galaxies with detected dust continuum, while inverse triangles represent upper limits on the dust mass. Dust evolution tracks are plotted for the constrained parameters [M_Gas, ini, η_out, η_in, ϵ_SN] ∼ [3.3, 0−2, 0.6, 0.1] and [4.4, 0−2, 0.6, 0.1] for the Chabrier and THIMF models, respectively, and for galaxy ages of 400 Myr, 800 Myr, and 1200 Myr for illustrative purpose. The solid color lines represent models assuming η_out = 0, while the dotted lines show the effect of increasing the outflow efficiency to η_out = 2. The models range from 25% dust condensation without dust growth in the ISM to 100% condensation with maximum dust growth efficiency. The galaxies are color-coded according to the age of their main stellar population.