Image Details
Caption: Figure 1.
PDFs of the stellar parameters of HD 33142 derived by applying the Bayesian inference scheme of Stock et al. (2018) and using the parallax, B and V photometry, and the spectroscopic metallicity estimate provided in Table 1. The vertical dashed lines show the 0.16, 0.5 (median), and 0.84 quantiles of the posterior samples.
© 2022. The Author(s). Published by the American Astronomical Society.