Image Details
Caption: Figure 6.
The original light curves (left subplot), Lomb–Scargle periodograms (middle subplot), and phase-folded light curves (right subplot) of each eclipsing binary star found in the NGC 381 region. The periods (p) and corresponding frequencies (f) are also shown in the subplots. Star IDs are given at the top of each plot.
© 2023. The Author(s). Published by the American Astronomical Society.