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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 6.

Three-planet RV-model phase curves. Top: RV phase curve of the massive and highly eccentric π Men b. Middle: RV phase curve of π Men c, a much smaller signal. Bottom: RV phase curve of π Men d, a signal of similar amplitude to π Men c, with a much wider period and higher eccentricity.

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