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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 2.

O – C plot of π Men c transit midpoints. Midpoints are designated by epoch, and differences are in units of minutes. The dotted black line traces the path of expected transit-midpoint values (in other words, the line where δtn = 0). We find our O – C plot to be consistent with a lack of TTVs.

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