TL;DR
ELLC is a new, fast, and flexible light curve model for analyzing detached eclipsing binary stars and transiting exoplanets, capable of handling complex effects and suitable for high-quality space-based data.
Contribution
The paper introduces ELLC, a novel light curve modeling tool that is accurate, versatile, and computationally efficient for detailed analysis of binary and exoplanet systems.
Findings
ELLC accurately models high-quality space photometry.
It effectively includes star spots, Doppler boosting, and light-travel time effects.
The model is fast enough for modern Monte Carlo data analysis.
Abstract
Very high quality light curves are now available for thousands of detached eclipsing binary stars and transiting exoplanet systems as a result of surveys for transiting exoplanets and other large-scale photometric surveys. I have developed a binary star model (ELLC) that can be used to analyse the light curves of detached eclipsing binary stars and transiting exoplanet systems that is fast and accurate, and that can include the effects of star spots, Doppler boosting and light-travel time within binaries with eccentric orbits. The model represents the stars as triaxial ellipsoids. The apparent flux from the binary is calculated using Gauss-Legendre integration over the ellipses that are the projection of these ellipsoids on the sky. The model can also be used to calculate the flux-weighted radial velocity of the stars during an eclipse (Rossiter-McLaughlin effect). The main features of…
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