Kepler-band model intensity profiles (black-solid) predicted for both plane-parallel (left) and spherically symmetric (right) model stellar atmospheres with Teff = 5000 K, log g = 2 and M = 10 M⊙. Along with the intensity profiles, best-fit linear (green-dashed), quadratic (orange-short-dashed), square-root (blue-dotted), four-parameter (violet-long-dash-dotted), logarithmic (brown-short-dash-dotted), and exponential (grey-double-dash) limb-darkening relations are plotted. Bottom panels show the difference, Δ ≡ Imodel − Ilaw, between model intensities and best-fit limb-darkening laws.
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