Image Details
Caption: Figure 5.
Histogram of all the candidates in each band, after the cross-correlation filter. They seem to prefer some frequencies to others, in a manner that is somewhat correlated with pink bands that are known to be heavily contaminated by RFI, from D. C. Price et al. (2019). The gray bands were completely excluded from our analysis.
© 2025. The Author(s). Published by the American Astronomical Society.