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• W2056545135 startingPage "A112" @default.
• W2056545135 abstract "Context. Planetary transit light curves are influenced by a variety of fundamental parameters, such as the orbital geometry and the surface brightness distribution of the host star. Stellar limb darkening (LD) is therefore among the key parameters of transit modeling. In many applications, LD is presumed to be known and modeled based on synthetic stellar atmospheres." @default.
• W2056545135 created "2016-06-24" @default.
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• W2056545135 date "2013-12-01" @default.
• W2056545135 modified "2023-10-14" @default.
• W2056545135 title "High-precision stellar limb-darkening measurements" @default.
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• W2056545135 doi "https://doi.org/10.1051/0004-6361/201322079" @default.
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