sM_Dust plotted against sSFR for the ALPINE galaxies assuming a Chabrier IMF (left) and THIMF (right). The circles represent galaxies with detected continuum emission, while the inverse triangles mark the upper limits on dust mass. The contributions from the various dust sources are distinguished by the different identifiers. The mass-loading factor ranges from 0 to 2. The overall dust evolution track, which includes all contributions, is shown 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 cases, respectively, at an age ∼ 1200 Myr (hatched region). The green, pink, and brown patches represent contributions from SNII, SNIa, and AGB stars, respectively. For SNII and SNIa, the models range from 25% dust condensation with η_out = 0, to 100% condensation with η_out = 2. For AGB stars, the models vary with η_out from 0 to 2. The blue patch shows the contribution of ISM growth to the total dust content, assuming a growth efficiency of 1, varying with η_out from 0 to 2. The galaxies are color-coded based on the age of their main stellar population.