Image Details
Caption: Figure 8.
MCMC mass (left) and effective temperature (right) posterior samples for HIP 17453 B from interpolation of the Sonora Diamondback (C. V. Morley et al. 2024) evolution model grid. We calculate the 68% HPDI of the posteriors to remove the influence of the low-probability peak at young ages and in the low-mass tail of the mass posterior.
© 2026. The Author(s). Published by the American Astronomical Society.