Fig. 13
56Ni mass distribution for SNe II (IIP and IIL, estimates from Hamuy 2003; Inserra et al. 2013; Anderson et al. 2014; and Rubin et al. 2015) in blue, and our SN 1987A-like SNe in green. 56Ni mass estimates that are based on at most two points on the radioactive tail are highlighted by dashed edges (red lines indicate upper limits, black lines mark lower limits).
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