  We present the first preliminary results on the analysis of ground-based time
series of the {\gamma} Dor star KIC 6462033 (TYC 3144-646-1, V = 10.83, P =
0.69686 d) as well as Kepler photometry in order to study pulsational behaviour
in this star.{\gamma} Dor variables, which exhibit g-mode pulsations, are
promising asteroseismic targets to understand their rich complexity of
pulsational characteristics in detail. In order to achieve this goal, intensive
and numerous multicolour and high resolution spectroscopic observations are
also required, to complete space-based data aimed at the determination of their
physical parameters.
