Cumulative distribution functions of ejecta masses, explosion energies, nickel masses, and kick velocities, separated for the full sample of models and separated between Type Ib and Ic SNe that result from analysing our core-collapse models with the Mandel & Müller (2020) model, weighted by the IMF from Salpeter (1955). Different colour lines represent different metallicities. The observed distributions of ejecta masses, explosion energies and nickel masses are drawn from Taddia et al. (2018) for Type Ib, IIb (grouped with Type Ib), and Ic SNe, and additionally from Barbarino et al. (2021) for a larger sample of Type Ic SNe. The average values of each distribution are indicated with vertical lines at the top of each panel.