E. Michel, A. Baglin, W. W. Weiss, M. Auvergne, C. Catala, C. Aerts, T. Appourchaux, C. Barban, F. Baudin, M. Briquet, F. Carrier, P. Degroote, J. De Ridder, R. A. Garcia, R. Garrido, J. Gutiérrez-Soto, T. Kallinger, L. Lefevre, C. Neiner, E. Poretti, R. Samadi, L. M. Sarro, G. Alecian, L. Andrade, J. Ballot, O. Benomar, G. Berthomieu, P. Boumier, S. Charpinet, B. de Batz, S. Deheuvels, M.-A. Dupret, M. Emilio, J. Fabregat, W. Facanha, M. Floquet, Y. Frémat, M. Fridlund, M.-J. Goupil, A. Grotsch-Noels, G. Handler, A. L. Huat, A.-M. Hubert, E. Janot-Pacheco, H. Kjeldsen, Y. Lebreton, B. Leroy, C. Martayan, P. Mathias, A. Miglio, J. Montalbán, M. J. P. F. G. Monteiro, B. Mosser, J. Provost, C. Regulo, J. Renan de Medeiros, I. Ribas, T. Roca Cortes, I. W. Roxburgh, J. Suso, A. Thoul, T. Toutain, D. Tiphène, S. Turck-Chièze, S. Vauclair, G. Vauclair, K. Zwintz

Abstract
About one year after the end of the first observational run and six months after the first  CoRoT data delivery, we comment the data exploitation progress for different types of  stars. We consider first results to illustrate how these data of unprecedented quality shed a new light on the field of stellar seismology.

Communications in Asteroseismology
Volume 156, Page 73
2008 December

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