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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 2.

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 left panel shows the one-dimensional GP fit to each available passband, and the right panel shows the two-dimensional GP fit to all of the passbands (shown in different colors). The two-dimensional GP infers the light curve in passbands where there are no (or few) observations, unlike the one-dimensional GP.

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