  We present the first results of a time-resolved CCD photometric and
time-series analysis of NSV 13601, a variable star of Pegasus constellation.
The 14" SCT of Maharaja Krishnakumarsinhji Bhavnagar University(MKBU) was used
for observations. Analysis was performed both in Vstar and Period04 software
and compared their results. The main results are as follows: From data
analysis, it's period, $\sim$77.784 d(MKBU Data V)(VStar), $\sim$77.632 d(MKBU
  Data Ic)(VStar), $\sim$77.058 d(MKBU Data V)(Period04) and $\sim$49.560
d(MKBU Data Ic)(Period04). It's V and I mean magnitudes for MKBU Data are
12.203 (V) and 11.292 (I) mag respectively. We confirm it as a variable star.
  \keywords{Stars: individual: NSV 13601 --- stars: oscillations ---
techniques: photometric.
