Bolometric luminosities for our SNe. Left: SN 2020jfo with some comparison objects (see text). The green solid lines with shaded regions are estimated with the Lyman et al. (2016) method and is a Gaussian Process fit to that LC. The blue region is a linear interpolation for the region with less data. The red fit on the plateau is for a diluted BB fit to our UV through NIR data, and matches the Lyman et al. method well on the later part of the plateau. Right: SNe 2020amv and 2020jfv. These were derived using the Lyman et al. method, which is rather approximate given the unusual nature of these SNe.