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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 7.

Histogram representations for the period–temperature distribution of TESS, with no photometric variability cut (top), and restricting to ﹩\mathrm{log}({R}_{\mathrm{per}}/\mathrm{ppm})\gt 3.5﹩ (bottom). Our polynomial fit to the Kepler period gap is shown by the gray bands in each histogram, with width of 5 days chosen only for visibility. Temperatures are from the TIC.

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