Using open-cluster gyrochronology as a constraint, the authors recover short stellar rotation periods from simulated and real blended TESS light curves, but periods beyond about 10 days generally remain unresolved.
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Evaluating the Limits of Rotation Period Recovery through Gyrochronology Criteria
Using open-cluster gyrochronology as a constraint, the authors recover short stellar rotation periods from simulated and real blended TESS light curves, but periods beyond about 10 days generally remain unresolved.