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The preliminary results of an analysis of the KIC 5390438 and KIC 5701829light curves are presented. The variations of these stars were detected byBaran et al. (2011a) in a search for pulsating M dwarfs in the Kepler publicdatabase. The objects have been observed by the Kepler spacecraft during the Q2and Q3 runs in a short-candence mode (integration time of $\sim$ 1 min). AFourier analysis of the time series data has been performed by using thePERIOD04 package. The resulting power spectrum of each star shows a clearexcess of power in the frequency range 100 and 350 $\mu$Hz with a sequence ofspaced peaks typical of solar-like oscillations. A rough estimation of thelarge and small separations has been obtained. Spectroscopic observationssecured at the Observatorio Astronomico Nacional in San Pedro M\'artir allowedus to derive a spectral classification K2III and K0III for KIC 5390438 and KIC5701829, respectively. Thus, KIC 5390438 and KIC 5701829 have been identifiedas solar-like oscillating red giant stars.

Solar like oscillations in the stars KIC 5390438 and KIC 5701829 observed by Kepler