The primary purpose of our study is to obtain rotational information for Koronis family members to be used in larger studies of the YORP effect. We have obtained photometry at the Union College Observatory (UCO) 0.5m telescope of Koronis family member (2498) Tsesevich from 2022 September - October. Standard corrections were applied for light travel time, unit distances, and solar phase angle. ATLAS data were included to provide a longer time span than that obtained at UCO. We present our composite light curve and compare it to published results from the 2021 apparition.
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