Image Details
Caption: Figure 4.
Fitted spectroscopic limb darkening coefficients for a quadratic limb darkening law and posteriors against uniform priors centered about the ExoTiC-LD MPS2 stellar grid model (solid lines). Due to the agreement between the predicted and fit values, we fixed the limb darkening coefficients to the predicted values from the MPS2 grid when fitting the spectroscopic light curves.
© 2026. The Author(s). Published by the American Astronomical Society.