Image Details
Caption: Figure 13.
WFD test-set recall (top two rows) and precision (bottom two rows) as a function of the length of the longest inter-night gap (left panels) and the number of observations between 10 days before and 30 days after the peak length (right panels), per SN class. In the first and third rows, we reproduce the results of this work previously shown in Figures 9 and 10. In the second and fourth rows, we show the classification predictions obtained by Boone (2019).
© 2022. The Author(s). Published by the American Astronomical Society.