Image Details
Caption: Figure 9.
PHOENIX model limb-darkening comparison as a function of ﹩{\mu }_{{\rm{\min }}}﹩. Top: offset in the linear coefficient, Δℓ, for each target. Middle: offset in the curvature coefficient, Δδ. Bottom: reduced chi-square (﹩{\chi }_{\nu }^{2}﹩) for each target (colored lines) and the aggregate statistics summing across all systems (black), shown both with and without offsets applied. Points are colored by stellar effective temperature.
© 2026. The Author(s). Published by the American Astronomical Society.