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The launch of the Kepler mission on 7th March 2009 opened a new bright futurefor the search of extra-solar planets while a huge amount of stars will beobserved leading to the opportunity to better understand stellar evolution.This will allow us to probe different regions in the HR diagram and put moreconstraints on the stellar models. Up to now the asteroseismic missions such asMOST and CoRoT were providing some solar-like stars at a very slow cadence. Butto study the several hundreds of solar-like oscillating stars that will beobserved during the Kepler survey phase, an analysis devoted to one star isimpossible if we want to have as much information as we can in a small periodof time. We describe here our pipeline, A2Z, which calculates the globalparameters of the stars (rotation period, mean large spacing of the acousticmodes, maximum amplitude of the modes), fits the modes globally, and estimatesthe radius and mass of the stars. This pipeline has been tested on simulatedstars and applied to real data from CoRoT.

An automatic pipeline analysing solar-like oscillating targets tested on CoRoT and simulated data