  Recent re-determination of stellar atmospheric parameters for a sample of
stars observed during the {\it Kepler} mission allowed to enlarge the number of
{\it Kepler} B-type stars. We present the detailed frequency analysis for all
these objects. All stars exhibit pulsational variability with maximum
amplitudes at frequencies corresponding to high-order g modes. Peaks that could
be identified with low-order p/g modes are also extracted for a few stars. We
identified some patters in the oscillation spectra that can be associated with
the period spacings that can result from the asymptotic nature of the detected
pulsational modes. We also tentatively confront the observed oscillation
characteristics with predictions from linear nonadiabatic computations of
stellar pulsations. For high-order g modes the traditional approximation was
employed to include the effects of rotation on the frequency values and mode
instability.
