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Paper: The Concept of Few-Parameter Modeling of Eclipsing Binary and Exoplanet Transit Light Curves
Volume: 496, Living Together: Planets, Host Stars and Binaries
Page: 176
Authors: Mikulášek, Z.; Zejda, M.; Pribulla, T.; Vavnko, M.; Qian, S.-B.; Zhu, L.-Y.
Abstract: We present a new, few-parameter phenomenological model of light curves of eclipsing binaries and stars with transiting planets. The model is able to fit the observed light curves with an accuracy better than 1% of their amplitudes. It can be used for appropriate descriptions of light curve shapes, classification, mid-eclipse time determination, and detailed period analyses.
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