PI: Andrew Boyle · University of North Carolina at Chapel Hill
The goal of this project is to generate light curves from the TESS space telescope for every bright star (TESS magnitude < 16) within 500 pc of Earth. I will use these light curves to measure stellar rotation periods for as many of these stars as possible. By measuring stellar rotation periods, I can identify young stars close to Earth, find new groups of young stars, and create a list of young stars around which to search for planets.
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Cumulative usage · Jul 2, 2025 – Jul 2, 2026
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