Image Details
Caption: Figure 3.
The MAROON-X RVs collected on calibrator star HD 3651 in 2024, with the RV model for the eccentric planet from R. Basant et al. (2025a) subtracted. It is obvious that there is a slope in the RV residuals, as well as a potential offset around the time of the temperature anomaly.
© 2025. The Author(s). Published by the American Astronomical Society.