  We have carried detailed time-resolved timing analysis of an intermediate
polar V709 Cas using the long-baseline, short-cadence optical photometric data
from the Transiting Exoplanet Survey Satellite. We found an orbital period of
5.3341 $\pm$ 0.0004 hr, a spin period of 312.75 $\pm$ 0.02 sec, and a beat
period of 317.93 $\pm$ 0.03 sec, which is similar to the earlier published
results. From the continuous high cadence data, we found that V709 Cas is a
disc overflow system with disc-fed dominance.
