  The aim of present work is extract and analyses the light curves of the stars
in the field of two clusters, NGC 1960 and DOLIDZE 14. The photometric
calibration is performed by comprehensive method of secondary standard
transformation and differential photometry using two comparison stars per
candidate variable star. The resultant light curves for each potential variable
star are displayed and their period analyzed by two different methods. The
period and classification of 18 discovered short periodic type variable stars
of NGC 1960 are discussed, which consist of four known variable stars and
fourteen new variable stars. In the case of DOLIDZE 14, four discovered
variables consist of one miscellaneous, one rotational, two $binary$ type
variable stars. In the case of NGC~1960, the 12 selected comparison stars
appear to be likely candidate for long periodic variability and 4 stars may be
standard stars. The variation in brightness of other twenty comparison stars is
non-pulsating with an irregular pattern. Membership analysis of variable stars
is performed using their distance, kinematic probability and location in
$(U-B)$ vs $(B-V)$ TCD. C-M diagrams were constructed to confirm the
evolutionary state of the new variable stars.
