Image Details
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).
© 2022. The Author(s). Published by the American Astronomical Society.