Asteroseismic results of Hare & Hound exercise with simulated COROT data

G. Berthomieu1, T. Appourchaux2 on behalf of the COROT Seismology Working Group
1 Département Cassini, UMR CNRS 6529, Observatoire de la Côte d'Azur, BP 4229, 06304 Nice Cedex4, France.
2 Space Science Department of ESA, ESTEC, P.O.Box 299, NL-2200AG Noordwijk, The Netherlands.

 

With the aim of preparing the interpretation of future COROT observations, a Hare and Hound exercise has been performed on a solar-like oscillating star. The methods used to construct simulated time series and to recover the properties of the star using the frequencies extracted from these time series are described and the comparison between the results and the theoretical inputs are presented

 
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