Photospheric activity and rotation of the planet-hosting star CoRoT-Exo-4a
A. F. Lanza, S. Aigrain, S. Messina, G. Leto, I. Pagano, M. Auvergne,, A. Baglin, P. Barge, A. S. Bonomo, A. Collier Cameron, G. Cutispoto, M., Deleuil, J. R. De Medeiros, B. Foing, C. Moutou

TL;DR
This study analyzes the surface rotation and activity of the star CoRoT-Exo-4a, hosting a hot Jupiter, revealing active longitudes, differential rotation, and potential star-planet magnetic interactions based on 58 days of optical observations.
Contribution
It introduces a maximum entropy spot modelling technique to analyze stellar activity and rotation, highlighting star-planet interactions in a transiting exoplanet system.
Findings
Identification of three main active longitudes with 30-60 day lifetimes.
Detection of quasi-synchronous rotation of active regions with the planet.
Evidence suggesting magnetic star-planet interaction near the subplanetary longitude.
Abstract
The space experiment CoRoT has recently detected a transiting hot Jupiter in orbit around a moderately active F-type main-sequence star (CoRoT-Exo-4a). This planetary system is of particular interest because it has an orbital period of 9.202 days, the second longest one among the transiting planets known to date. We study the surface rotation and the activity of the host star during an uninterrupted sequence of optical observations of 58 days. Our approach is based on a maximum entropy spot modelling technique extensively tested by modelling the variation of the total solar irradiance. It assumes that stellar active regions consist of cool spots and bright faculae, analogous to sunspots and solar photospheric faculae, whose visibility is modulated by stellar rotation. The modelling of the light curve of CoRoT-Exo-4a reveals three main active longitudes with lifetimes between about 30…
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