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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 18.

The 6 hr CDPP of our TESS-SPOC “pure noise” light curves (black points), which are taken from hot stars observed in the SCVZ during TESS Cycle 1, and a subsample of cool-star target light curves (red points). The photometric noise properties are virtually identical for the two samples.

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