An automated pipeline for asteroseismology based on the autocorrelation of stellar time series
arXiv:1006.5079
Abstract
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.
Proceedings of the HELAS workshop New insights into the Sun held in Ponte de Lima, 09/2009