Image Details
Caption: Figure 9.
WFD test-set recall (left panels) and precision (middle panels) as a function of the number of gaps longer than 10 days (top row) and the length of the longest inter-night gap (bottom row), per SN class. We only included events with median inter-night gap <3.5 days and light curves between 50 and 175 days long. These results show that large gaps do not significantly impact the SNe classification for this subset. The right panel shows the density of events as a function of the number of large gaps (top row) and the length of the longest inter-night gap (bottom row). We note that the results in the tails of the distribution are dominated by small number effects.
© 2022. The Author(s). Published by the American Astronomical Society.