Border variability of transit light-curves

Author(s)
Maxim Khodachenko, Oleksiy Arkhypov, Manuel Güdel
Abstract

A model-independent method for detection of transit borders, using the polynomial approximation of the light-curve parts, is proposed. The trial processing of long-cadence light-curves of 183 Kepler's exoplanets reveals for some objects a variability of transit's start/end- times and asymmetry. The diagnostic diagram was constructed for preliminary classification and interpretation of such results.

Organisation(s)
Department of Astrophysics
External organisation(s)
Österreichische Akademie der Wissenschaften (ÖAW)
Volume
13
Publication date
09-2019
Austrian Fields of Science 2012
103003 Astronomy, 103004 Astrophysics
Portal url
https://ucrisportal.univie.ac.at/en/publications/a86dad67-f80b-4312-9806-53ea2bef5bbc