Time evolution of the disk mass, M_disk, of our models. Colors indicate the viscous alpha, α_visc, of the models. The black boxes show which stellar mass, and therefore accretion rate, was used to calculate the initial disk mass of the models (see Table 1). We note that we exclude models with α_visc = 10⁻² for M_* = [0.32, 1.0] M_⊙ as the gas disk sizes of these models can be ruled out by observations of disks in Lupus (Trapman et al. 2020). We also note that models with M_* = 1.0 M_⊙ and α_visc = 10⁻⁴ are much more massive (M_gas ≳ 2 × 10⁻¹ M_⊙) than the disks observed in Lupus (cf. Ansdell et al. 2016; see Fig. A.1 in Trapman et al. 2020).