The TESS All-Sky Rotation Survey: Periods for 1,046,317 Stars Within 500 pc
Andrew W. Boyle, Luke G. Bouma, Andrew W. Mann

TL;DR
The TESS All-Sky Rotation Survey (TARS) provides rotation periods for over one million stars within 500 pc, significantly expanding the available data for stellar evolution and Galactic studies.
Contribution
This work delivers the largest homogeneous catalog of stellar rotation periods from TESS data and introduces a method to recover long periods reliably from single sectors.
Findings
Catalog includes 1,046,317 stars with estimated 93% rotation periods.
Increases rotation period data for stars within 100 pc by 2.3 times.
Reliable recovery of periods up to 25 days from a single TESS sector.
Abstract
Stellar rotation is a fundamental tracer of stellar magnetic evolution, age, and activity, with broad implications for Galactic archaeology and exoplanet characterization. The Transiting Exoplanet Survey Satellite (TESS) provides high-precision time-series photometry across the sky, enabling rotation measurements for an unprecedented number of stars. We present the TESS All-Sky Rotation Survey (TARS), an all-sky catalog of stellar variability periods for 1,046,317 stars with T < 16 and distances within 500 pc. We estimate that 93% of these periods are rotation periods. This catalog increases the number of rotation period measurements for stars with T < 16 within 100 pc by a factor of 2.3 and within 500 pc by 4.0. We also present a method to correct half-period aliases in TESS data and show that it reliably recovers periods as long as 25 days from a single TESS sector. TARS represents…
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