Time evolution of the rate of Type Ia SNe, Type II SNe, MR-SNe, and MNS (upper-left panel); SFR (upper-right panel); surface densities of gas (lower-left panel); and stars (lower-right panel) as predicted by the three-infall model. Predictions of the model are compared to present day values from Cappellaro et al. (1999) (for SNe rates), from Abbott et al. (2021) (for MNS rate) and from Prantzos et al. (2018) (for SFR and surface gas and stars densities).