pith. sign in

arxiv: 1502.07477 · v1 · pith:6JONNFCSnew · submitted 2015-02-26 · 🌌 astro-ph.SR

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

classification 🌌 astro-ph.SR
keywords lightcurveseclipsingfew-parametermodelableaccuracyamplitudes
0
0 comments X
read the original abstract

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.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.