Using limb darkening to measure fundamental parameters of stars

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Fig. 5

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V-band values of the A limb-darkening coefficient (top panel) and the B limb-darkening coefficient (bottom panel) for the linear-plus-square-root parametrization given by Eq. (2), plotted as a function of the extension parameter, R_⋆/M_⋆ in solar units. The symbols have the same meaning as in Fig. 2.

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