Image Details
Caption: Figure B2.
Posterior slope overlap probabilities for the values of α derived from the bootstrap fits to [X/H] versus [Fe/H] for the benchmark M dwarf (solid black) and FGK (solid orange) samples. Included are also the distributions for the M dwarf samples from F. Jahandar et al. (2025) (dotted green) and J. Maldonado et al. (2020) (dashed blue).
© 2026. The Author(s). Published by the American Astronomical Society.