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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 3.

Systematics masquerade as period detections. Top: the period of the highest peak in the Lomb–Scargle (L-S) periodogram across all TESS sectors. The sinusoidal structures across sectors are harmonics of the TESS data gap. Bottom left: our systematics classifier identifies and separates systematics from other rotation signals. The systematics classifier is trained so rotation measurements with a high probability are more likely to be real signals and less likely to be a systematic. Sector 6 experienced momentum dumps every 3.125 days. The blue and gray stars show the L-S period and power of the two light curves in the bottom-right panel. Bottom right: TIC 231925886 and TIC 302869120 both have L-S peak periods of ∼2.9 days in Sector 6, but TIC 231925886 has a systematics classifier score of 1.0 (high probability of being a rotation signal) while TIC 302869120 has a systematics classifier score of 0.0 (high probability of being a systematic).

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