SuperBol (Nicholl 2018) pseudo-bolometric light curve of the second peak integrated over observed bands (black open circles), and a bolometric light curve based on blackbody fits (red filled circles), highly uncertain before the rebrightening. The difference is notable only around maximum light. The late-time decline is inconsistent with ⁵⁶Co decay (solid black line). Pseudo-bolometric light curves of SNe 1998bw (Patat et al. 2001), 2019cad (Gutiérrez et al. 2021), 2022jli (Moore et al. 2023), and 2022xxf (Kuncarayakti et al. 2023) are included for comparison.