Bolometric light curves and velocity profiles for our sample. For the SNe without velocity measurements, we assumed the average velocity profile. The bolometric light curves were fit with the Arnett model, shown as a solid line. The velocity profiles were fit with a scaled polynomial that also reproduces the velocity profile of the SN Ic spectral templates provided by Modjaz et al. (2016), and it is shown with solid lines in the velocity subpanels. The velocity at peak brightness is marked with an empty diamond.