Image Details
Caption: Figure 6.
Stellar activity indicators for TOI-4468 measured by NEID: the chromatic index (CRX) and differential line width (dLW). There appears to be some evidence of variation in dLW on the same period as the RV signal attributed to TOI-4468.03. Without more data, however, we cannot verify whether the additional RV signal is due to stellar activity or to a third planet in the system.
© 2026. The Author(s). Published by the American Astronomical Society.