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Paper: Transit and Spectral Studies of CoRoT-2
Volume: 448, 16th Cambridge Workshop on Cool Stars, Stellar Systems, and the Sun
Page: 1043
Authors: Wolter, U.; Czesla, S.; Schröter, S.; Huber, K.; Schmitt, J. H. M. M.
Abstract: A transiting planet acts as a sharply defined shutter that scans the surface of its host star. Based on very-low-noise photometry from the CoRoT satellite and high-resolution spectra taken with VLT/UVES we employ this shutter to resolve surface features of the highly active G-type star CoRoT-2a which is transited by the planet CoRoT-2b. We shortly discuss the age of the CoRoT-2 system based on the equivalent width of the Li I λ 6708 Å line of 140 ± 1 mÅ.
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