Image Details
Caption: Figure 8.
Panel (a) shows the RVs for TOI-3984 A derived with modified versions of SERVAL. Panel (b) displays the phase-folded RVs plotted with model posteriors and the residuals to the fit. In panels (a) and (b), the dashed line is the best-fitting Keplerian model. The shaded regions denote the 1σ (darkest), 2σ, and 3σ (lightest) extent of the model posteriors. The modeling is described in Section 4.
© 2023. The Author(s). Published by the American Astronomical Society.