On 6,730 simulated LSST supernova light curves, the authors find that survey photometry alone recovers progenitor mass reasonably but estimates explosion energy and nickel mass with large errors.
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Core-collapse supernova parameter estimation with the upcoming Vera C. Rubin Observatory
On 6,730 simulated LSST supernova light curves, the authors find that survey photometry alone recovers progenitor mass reasonably but estimates explosion energy and nickel mass with large errors.