  The private Lookout Observatory (LO) monitored the classic nova V1112 Persei
on 37 nights spanning over 80 days, beginning shortly after its discovery by
Seiji Ueda on 25 Nov 2020. Images were captured at a high cadence, with
exposure lengths of initially less than 2 seconds and with some sessions
lasting more than ten hours. The standard error of the photometry was typically
better than 5 thousandths of a magnitude (5 mmag). This cadence and precision
allowed for not only the observation of the expected dimming of the nova, but
also variability having a period of 0.608 +- 0.005 days. This data compliments
the publicly available photometry from the American Association of Variable
Star Observers (AAVSO) and the resultant data is combined to perform this
photometric analysis. This paper does not attempt an in-depth physical analysis
of the nova from an astrophysical perspective.
