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Characteristics of solar-like oscillations in red giants observed in the CoRoT exoplanet field
<i>Context. <i/>Observations during the first long run (~150 days) in the exo-planet field of CoRoT increase the number of G-K giant stars for which solar-like oscillations are observed by a factor of 100. This opens the possibility to study the characteristics of their oscillations in a statistical sense.<i>Aims. <i/>We aim …