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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 8.

WFD test-set recall (left panel) and precision (middle panel) as a function of median inter-night gap per SNe class for events with light curves between 50 and 175 days long. In general, the recall and precision are higher for events whose median inter-night gap is <3.5 days (left side of the black line). The right panel shows the density of events as a function of median inter-night gap; ∼64% of SNe Ia, ∼63% of SNe Ibc, and ∼66% of SNe II from the test-set events have median inter-night gap <3.5 days and light-curve lengths between 50 and 175 days.

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