  Since 1992, observations of roAp stars have been carried out using the
dual-channel photometer attached to the 0.8m telescope, which is situated in
Central Asia, at the Mt. Dushak-Erekdag station of Odessa Astronomical
Observatory. Some results of observations of gamma Equ and of HD 134214 are
presented. 5 stars were investigated as roAp candidates. The Fourier spectra of
4 stars did not show any variability in the high-frequency region. The Fourier
spectrum of HD 99563 revealed a peak at a frequency f=128.9 c/d and with a
semi-amplitude of 3.98 mmag.
