  This paper presents the detection of a periodic dimming event in the
lightcurve of the G1.5IV-V type star KIC 1718360. This is based on
visible-light observations conducted by both the TESS and Kepler space
telescopes. Analysis of the data seems to point toward a high rotation rate in
the star, with a rotational period of 2.938 days. The high variability seen
within the star's lightcurve points toward classification as a rotating
variable. The initial observation was made in Kepler Quarter 16 data using the
One-Class SVM machine learning method. Subsequent observations by the TESS
space telescope corroborated these findings. It appears that KIC 1718360 is a
nearby rotating variable that appears in little to no major catalogs as such. A
secondary, additional periodic dip is also present, indicating a possible
exoplanetary companion.
