A grid of 5,346 supernova models fitted to eleven type IIP supernovae recovers progenitor and nickel masses with precision comparable to progenitor imaging and yields a typical explosion energy of 10^50.52 erg.
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Supernova lightCURVE POPulation Synthesis II: Validation against supernovae with an observed progenitor
A grid of 5,346 supernova models fitted to eleven type IIP supernovae recovers progenitor and nickel masses with precision comparable to progenitor imaging and yields a typical explosion energy of 10^50.52 erg.