TL;DR
This paper introduces an efficient method for sampling limb-darkening coefficients of a three-parameter law, enabling more accurate modeling of stellar limb-darkening effects in astronomical observations.
Contribution
It presents a novel, fast sampling technique for three-parameter limb-darkening coefficients using a cone transformation, improving over previous two-parameter methods.
Findings
Uniform samples are physically valid in 97.3% of cases.
The method covers 94.4% of the allowed parameter space.
Provides open-source code for sampling and validation.
Abstract
Stellar limb-darkening impacts a wide range of astronomical measurements. The accuracy to which it is modelled limits the accuracy in any covariant parameters of interest, such as the radius of a transiting planet. With the ever growing availability of precise observations and the importance of robust estimates of astrophysical parameters, an emerging trend has been to freely fit the limb-darkening coefficients (LDCs) describing a limb-darkening law of choice, in order to propagate our ignorance of the true intensity profile. In practice, this approach has been limited to two-parameter limb-darkening laws, such as the quadratic law, due to the relative ease of sampling the physically allowed range of LDCs. Here, we provide a highly efficient method for sampling LDCs describing a more accurate three-parameter non-linear law. We first derive analytic criteria which can quickly test if a…
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