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Having started science operations in May 2009, the Kepler photometer has beenable to provide exquisite data of solar-like stars. Five out of the 42 starsobserved continuously during the survey phase show evidence of oscillations,even though they are rather faint (magnitudes from 10.5 to 12). In this paper,we present an overview of the results of the seismic analysis of 4 of thesestars observed during more than eight months.

Seismic analysis of four solar-like stars observed during more than eight months by Kepler