Image Details
Caption: Figure 6.
RV measurements of TOI-7154 from 20 spectroscopic observations with PARAS-2 (black points) and 8 spectroscopic observations with TRES (green squares) are shown as a function of time (left panel). The same RV data are shown as a function of the orbital phase (right panel). In both panels, the best-fit RV model obtained using EXOFASTv2 is shown by the red curve, while the residuals between the model and the observations are displayed in the corresponding lower panels.
© 2026. The Author(s). Published by the American Astronomical Society.