  We study the binary corrected X-ray light curve of Cygnus X-3 using the
RXTE-ASM data and RXTE-PCA data. We find that the X-ray template derived from
the EXOSAT observations adequately explains the binary variations. Using the
recently determined quadratic binary ephemeris we correct the RXTE-PCA
lightcurve and obtain the power spectrum which shows distinct features of
shifting towards the low frequency regime vis-a-vis the Galactic X-ray
binaries. The power spectrum doesn't vary from the hard to the soft state. We
also obtain the binary corrected RXTE-ASM monitoring lightcurve and examine the
previously obtained correlation between soft X-ray (2-12 keV from RXTE-ASM),
hard X-ray (20-100 keV from CGRO-BATSE) and radio (2.2 GHz from GBI) after the
binary correction. We find that the correlation time scale is less than a day.
