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An automated pipeline for asteroseismology based on the autocorrelation of stellar time series

The autocorrelation of an asteroseismic time series has been identified as a powerful tool capable of providing measurements of the large frequency separations. The performance of this method has been assessed and quantified by Mosser & Appourchaux (2009). We propose now an automated pipeline based on it and describe its performance.

preprint2010arXivOpen access

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