Image Details
Caption: Figure 18.
Comparison between TESS (red), ASAS-SN (green and blue), and ZTF (cyan, magenta, and green, for the zg, zr, and zi bands, respectively) photometry for the several quadruple candidates. The ground-based photometry is binned for clarity. First row: both primary and secondary eclipses seen for one component of the respective quadruple candidate. Second row: both primary and secondary seen for both components. Third row: both EBs are present in ZTF but neither in ASAS-SN. Last row: both EBs present in ZTF but only one or the other in ASAS-SN.
© 2025. The Author(s). Published by the American Astronomical Society.