Image Details
Caption: Figure 6.
JWST-fit quadratic limb-darkening coefficient spectra for WASP-121, WASP-94, and HAT-P-11, compared with stellar-atmosphere model predictions using ﹩{\mu }_{{\rm{\min }}}=0.2﹩. The empirically derived coefficients ℓ (limb intensity) and δ (curvature) are shown with 1σ uncertainties. Model predictions from PHOENIX, MPS-ATLAS (sets 1 and 2), and Stagger are shown both with (solid) and without (dashed) the recommended offsets applied.
© 2026. The Author(s). Published by the American Astronomical Society.