Image Details
Caption: Figure 9.
Zoom-in RV plots for Figure 8 with the same legend. The rms values are calculated for each observing night and displayed respectively in each subplot. Nights 1–3 and nights 23–27 are each modeled with a GP kernel but fitted with a joint likelihood to share the same set of hyperparameters for the GP, which is done to effectively accommodate the long gap in the baseline.
© 2026. The Author(s). Published by the American Astronomical Society.