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Measuring Long Stellar Rotation Periods (>10 days) from TESS FFI Light Curves is Possible: An Investigation Using TESS and ZTF

  • Authors: Soichiro Hattori, Ruth Angus, Daniel Foreman-Mackey, Yuxi (Lucy) Lu, Isabel Colman

Soichiro Hattori et al 2025 The Astronomical Journal 170 .

  • Provider: AAS Journals

Caption: Figure 6.

A plot comparing the periods measured from the ZTF light curves and the TESS light curves. The points are colored by their TESS peak powers. The 1:1 line with 10% uncertainties are indicated with the black line and the shaded region. The 1:2 line is indicated in red. A potential Lomb–Scargle failure mode caused by the window function of the TESS observing sector is indicated as a dashed blue line (more description in text).

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