Tidal tails of stellar clusters are important laboratories for the evolution of stellar populations and the Milky Way at large. Recent data from the Gaia mission has allowed identification of new tidal tail structures thanks to its high-precision astrometric data. One such tidal tail belongs to the Hyades, recently detected by Jerabkova et al. (2021). However, Gaia data alone is not enough to robustly confirm tail membership. In this work, we aim to confirm the coeval status of stars in the newly identified Hyades tidal tail through the use of gyrochronology, which infers stellar ages from their rotation rates. We also present `michael`, a means of measuring spot rotation using tried-and-tested methods from TESS Full Frame Images. Gyrochronology stands to be an important contributor to age-based studies in the era of Gaia DR3, PLATO asteroseismology and beyond, which accessible TESS rotation rates will help facilitate.