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Paper detail

The Concept of Few-Parameter Modelling of Eclipsing Binary and Exoplanet Transit Light Curves

We present a new few-parameter phenomenological model of light curves of eclipsing binaries and stars with transiting planets that is able to fit the observed light curves with the accuracy better than 1\% of their amplitudes. The model can be used namely for appropriate descriptions of light curve shapes, classification, mid-eclipse time determination, and fine period analyses.

preprint2015arXivOpen access
Zdeněk MikulášekMiloslav ZejdaTheodor PribullaMartin VaňkoShen-Bang QianLi-Ying Zhu
astro-ph.SR
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Zdeněk MikulášekMiloslav ZejdaTheodor PribullaMartin VaňkoShen-Bang QianLi-Ying Zhu

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