Bolometric LC (left) and photospheric velocity (right) comparison of N = 100 SuperSNEC models (blue lines) to SN 2011dh (top), SN 1993J (middle), and SN 2020oi (bottom) data (black markers). Velocities for SN 2011dh and SN 1993J are Fe II λ5169 absorption-minimum measurements; SN 2020oi uses Si I λ10460 as Fe II λ5169 could not be reliably measured. Observational data: SN 2011dh bolometric LC from M. Ergon et al. (2014, 2015), velocities from G. H. Marion et al. (2014); SN 1993J bolometric LC constructed from M. W. Richmond et al. (1994) photometry with UV/IR blackbody corrections, velocities measured from UNLV SN Archive spectra (R. Barbon et al. 1995); SN 2020oi bolometric LC constructed from the J. Rho et al. (2021) optical photometry using a blackbody bolometric correction, with Si I λ10460 velocities also from J. Rho et al. (2021).