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The TESS All-Sky Rotation Survey: Periods for 1,046,317 Stars within 500 pc

  • Authors: Andrew W. Boyle, Luke G. Bouma, Andrew W. Mann

Andrew W. Boyle et al 2026 The Astrophysical Journal Supplement Series 284 .

  • Provider: AAS Journals

Caption: Figure 4.

Systematics classifier performance vs. rotation period. Top left: reliability, defined as the fraction of random forest-selected signals that yield rotation periods consistent across >5 sectors, shown for several random forest probability thresholds. The classifier returns reliable detections across the full period range. Top right: completeness, defined as the fraction of all signals in the class that exceed the random forest probability threshold cuts. Completeness remains high for Prot ≲ 10 days, but decreases at longer periods. These panels suggest that the systematics classifier is reliable at longer periods; however, the yield of such measurements declines beyond ∼10–13 days. Bottom left: the reliability of the negative class as a function of Ssignal. Bottom right: the completeness of the negative class as a function of Ssystematic.

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