Rise times and peak absolute magnitudes of the PISN and SLSN models in the rest frame in the I_E band. The PISN models (R250, R225, R200, R175, R150, He130, He120, He110, He100, and He090) are from Kasen et al. (2011) and the SLSN template is from Moriya et al. (2022). We also show rise times and peak absolute magnitudes of the SN Ia template from Hsiao et al. (2007) and the SN II Nugent template for comparison (see Sect. 5 for details). The error bars in the SLSN, SN Ia, and SN II templates show a typical dispersion (e.g., Richardson et al. 2014; Miller et al. 2020; González-Gaitán et al. 2015).