Fig. 13

The decline parameter Δm15 computed for the bolometric light curves versus the late-time linear decay slope (top panel) and the peak bolometric magnitude (bottom panel). A possible correlation is observed in the first case, which might be explained by a range of values of the EK/Mej ratio (see Sect. 5). SNe IIb, Ib, Ic, and Ic-BL are represented in green, blue, red, and magenta, respectively.
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