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Considerations for Optimizing the Photometric Classification of Supernovae from the Rubin Observatory

  • Authors: Catarina S. Alves, Hiranya V. Peiris, Michelle Lochner, Jason D. McEwen, Tarek Allam, Rahul Biswas

Catarina S. Alves et al 2022 The Astrophysical Journal Supplement Series 258 .

  • Provider: AAS Journals

Caption: Figure 7.

WFD test-set recall (left panel) and precision (middle panel) as a function of light-curve length per SNe class. The right panel shows the density of events as a function of light-curve length. Because of the low number of events in the tails of the distribution, we restrict our analysis to between 50 and 175 days (comprising 94% of the events). Recall and precision increase for longer light curves.

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