Fig. 10.
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Angle averaged bolometric and UBVRI band light curves for a subset of our PGCD models. Observed light curves representing different subclasses of SNe Ia are also included. SN 1991T (Lira et al. 1998), SN 2011fe (Richmond & Smith 2012; Tsvetkov et al. 2013; Munari et al. 2013; Brown et al. 2014; Stahl et al. 2019) and SN 2012Z (Stritzinger et al. 2015; Brown et al. 2014; Stahl et al. 2019). We made use of the Open Supernova Catalogue (Guillochon et al. 2017) to obtain the observed photometry.
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