Image Details
Caption: Figure 3.
Observed RVs of WASP-193 from HARPS and PFS, phase folded to the orbital period of WASP-193 b, excluding those measurements taken during the planet’s transit. A relative RV offset between the two instruments has been removed. The best-fitting RV model is plot as the red line, while open circles show the data binned by orbital phase.
© 2025. The Author(s). Published by the American Astronomical Society.