Image Details
Caption: Figure 6.
Lomb–Scargle power spectrum of the TESS light curve of Paloma, with the two sets of frequency identifications proposed by Schwarz et al. (2007). The usage of “Case A” and “Case B” matches that of Schwarz et al. (2007). For the Case A identifications, there would be no appreciable signal at either ω or ω − Ω. For reasons discussed in the text, we prefer the “Case B” identifications.
© 2023. The Author(s). Published by the American Astronomical Society.