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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 4.

The left panel shows an SN Ibc light curve where the points show the observations, along with their error bars, and the lines and the shaded regions show the mean and standard deviation of the GP fit, respectively. The right panel shows a synthetic event at a different redshift generated from the original event using the procedure described in Section 4. Note that, in this example, the original event was simulated in the higher-cadence DDF survey, and we generated the synthetic event in the WFD survey.

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