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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 1.

A selection of TESS-SPOC simple aperture photometry light curves for which we successfully estimated rotation periods using the neural network. Top: an M dwarf with strong, coherent spot modulation. Middle: a slowly rotating M dwarf with several missing sectors. Bottom: a rapidly rotating G dwarf.

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