Image Details
Caption: Figure 3.
The left panel displays the relative position angle vs. time, shown with the maximum-likelihood orbital solution from the joint astrometric and RV fit (black curve). Residuals relative to the best-fit model are shown. The right panel shows relative separation vs. time, again compared with the maximum-likelihood orbital model. Fifty random orbits drawn from the posterior distribution are overplotted, which are colored by companion mass, and they are hidden behind the maximum-likelihood orbit.
© 2026. The Author(s). Published by the American Astronomical Society.