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TESS Photometry and Radial-velocity Analysis of the Sub-Neptune Exoplanet π Mensae c and the Wider π Mensae Planetary System

  • Authors: Skylar S. Larsen, Jake D. Turner, Nikole K. Lewis, Maryame El Moutamid, Diana Solano-Oropeza, Lili Alderson, V. Abby Boehm, Daniel A. Yahalomi, Emily K. Deibert, Ray Jayawardhana, Dong Lai, Adam B. Langeveld, Kyle A. Pearson

Skylar S. Larsen et al 2026 The Astronomical Journal 172 .

  • Provider: AAS Journals

Caption: Figure 4.

A frequency Lomb–Scargle periodogram of the π Men c O – C plot. The false-alarm probabilities (FAP) = 0.1, 0.05, and 0.01, measurements conditioned on the assumption of the null hypothesis of no signal, are shown as horizontal lines. Note that none of the periodogram peaks rise above any of the FAP thresholds, and as such, our O – C plot is consistent with a lack of TTVs.

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