  NASA's TESS mission \citep{tess} has produced high precision photometry of
millions of stars to the community. The majority of TESS observations have a
duration of $\approx$27 days, corresponding to a single observation during a
TESS sector. A small subset of TESS targets are observed for multiple sectors,
with approximately 1-2\% of targets falling in the Continuous Viewing Zone
(CVZ) during the prime mission \citep{yield}, where targets are observed
continuously for a year. These targets are highly valuable for extracting long
period rotation rates, which can be linked to stellar ages. We present a pip
installable Python tool for extracting long period rotation rates in the TESS
CVZ, while simultaneously mitigating instrument systematics.
