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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 11.

Distribution of the GP errors resulting from extrapolating GP fits to u or y passbands. F true is the true flux of an observation, and F predicted and σ predicted are the flux and its uncertainty, respectively, predicted by a GP fit at the corresponding epoch and passband. An ideal error estimation results in a unit Gaussian (black line).

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