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doi: 10.32023/0001-5237/69.3.1 | Vol. 69 (2019), No. 3 | pp. 205-226 |
CoRoT-18 b: Analysis of High-Precision Transit Light Curves with Starspot Features
St. Raetz1,2,3, A.M. Heras3, P. Gondoin4, M. Fernández5, V. Casanova5, T.O.B. Schmidt6 and G. Maciejewski7
1Institute for Astronomy and Astrophysics Tübingen (IAAT), University of Tübingen, Sand 1, D-72076 Tübingen, Germany
e-mail:raetz@astro.uni-tuebingen.de
2Freiburg Institute of Advanced Studies (FRIAS), University of Freiburg, Albertstraße 19, D-79104 Freiburg, Germany
3Science Support Office, Directorate of Science, European Space Research and Technology Centre (ESA/ESTEC), Keplerlaan 1, 2201 AZ Noordwijk, The Netherlands
4Future Missions Department, Directorate of Science, European Space Research and Technology Centre (ESA/ESTEC), Keplerlaan 1, 2201 AZ Noordwijk, The Netherlands
5Instituto de Astrofísica de Andalucía, CSIC, Apdo. 3004, 18080 Granada, Spain
6Hamburger Sternwarte, Gojenbergsweg 112, D-21029 Hamburg, Germany
7Centre for Astronomy, Faculty of Physics, Astronomy and Informatics, Nicolaus Copernicus University, Grudziadzka 5, 87-100 Toru�, Poland
Received: April 12, 2019
ABSTRACT
When a planet occults a spotty area on a stellar surface, the flux increases and a characteristic feature in a light curve - a bump - is observed. Among the planets detected by the CoRoT-mission CoRoT-18 is especially interesting as it exhibited spot crossings that we have analyzed in detail. We used four ground-based observations obtained at a 1.5-m telescope in Spain and the 13 available CoRoT-transits to refine and constrain stellar, planetary and geometrical parameters of the system. We found that the derived physical properties slightly deviate from the previously published values, most likely due to the different treatment of the stellar activity.
Following of a spot over several transits enabled us to measure the
stellar rotation period and the spin-orbit alignment. Our derived
values of Prot=5.19±0.03 d and
λ=6±13° are in agreement with the literature values
that were obtained with other methods. Although we cannot exclude a
very old age for CoRoT-18, our observations support the young star
hypothesis and, hence, yield constraints on the time-scale of planet
formation and migration.
Key words:
Planets and satellites: individual: CoRoT-18b - Stars: individual: CoRoT-18 - planetary systems
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