Image Details
Caption: Figure 14.
Secondary radius vs. host stellar mass for low-mass stars hosting confirmed exoplanets, TOIs, and candidates identified in B23. Colored by disposition as described for Figure 13. The previously assumed position of NGTS-EB-8 when it was described as a planet candidate in S. M. O’Brien et al. (2024) is plotted as an unfilled magenta star, and the position of NGTS-EB-8 as determined by the high k-range model from this work is shown as a filled cyan star.
© 2025. The Author(s). Published by the American Astronomical Society.