Limb-darkening offsets persist in lower-metallicity Sun-like stars in EBLM binaries, and M-dwarf companions are about 2.6% larger than MIST model predictions.
249, Exoplanets: Detection, Formation and Dynamics
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The EBLM project -- XIV. TESS light curves for eclipsing binaries with very low mass companions
Limb-darkening offsets persist in lower-metallicity Sun-like stars in EBLM binaries, and M-dwarf companions are about 2.6% larger than MIST model predictions.