Image Details
Caption: Figure 12.
WFD test-set recall (top two rows) and precision (bottom two rows) as a function of light-curve length (left panels), median inter-night gap (middle panels), and number of gaps larger than 10 days (right panels), per SN class. In the first and third rows, we reproduce the results of this work previously shown in Figures 7, 8, and 9. 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.