  The preliminary results of an analysis of the KIC 5390438 and KIC 5701829
light curves are presented. The variations of these stars were detected by
Baran et al. (2011a) in a search for pulsating M dwarfs in the Kepler public
database. The objects have been observed by the Kepler spacecraft during the Q2
and Q3 runs in a short-candence mode (integration time of $\sim$ 1 min). A
Fourier analysis of the time series data has been performed by using the
PERIOD04 package. The resulting power spectrum of each star shows a clear
excess of power in the frequency range 100 and 350 $\mu$Hz with a sequence of
spaced peaks typical of solar-like oscillations. A rough estimation of the
large and small separations has been obtained. Spectroscopic observations
secured at the Observatorio Astronomico Nacional in San Pedro M\'artir allowed
us to derive a spectral classification K2III and K0III for KIC 5390438 and KIC
5701829, respectively. Thus, KIC 5390438 and KIC 5701829 have been identified
as solar-like oscillating red giant stars.
