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TESS Stellar Rotation up to 80 Days in the Southern Continuous Viewing Zone

  • Authors: Zachary R. Claytor, Jennifer L. van Saders, Lyra Cao, Marc H. Pinsonneault, Johanna Teske, Rachael L. Beaton

Zachary R. Claytor et al 2024 The Astrophysical Journal 962 .

  • Provider: AAS Journals

Caption: Figure 5.

Period comparisons for the 427 stars in both the TESS-SPOC and TASOC samples. The solid black line represents perfect agreement, while the dashed red lines are ±50% error. The black dotted lines are at 27 days on either axis, showing the TESS sector length. There is generally good agreement for most stars, with a median percent error of 7%, and most of the disagreeing estimates have relatively large uncertainty. We note that while we do not include periods greater than 80 days in our analysis or table, we show them here to illustrate at what periods the agreement worsens.

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