Image Details
Caption: Figure 10.
TRES RV measurements of TOI-7019 showing the motion induced by the transiting BD. The best-fit model (black line) yields a semiamplitude of K = 4417 ± 17 m s−1, corresponding to a companion mass of 61.3MJ ± 2.1MJ. The top panel shows the RV time series phase-folded to the orbital period of the BD, while the bottom panel shows the full RV time series. The center-of-mass velocity ﹩{\mu }_{{\rm{TRES}}}﹩ has been subtracted from the TRES RVs in this figure.
© 2026. The Author(s). Published by the American Astronomical Society.