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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 8.

The logarithmic instellation (normalized to Earth) versus escape velocity of 564 cataloged exoplanets. JWST targets as of Cycle 5 are highlighted in red, while our π Men c measurements and propagated uncertainties are in orange. Earth’s position on this relation is designated as a blue star. The size of each point corresponds to its transmission-spectroscopy metric (TSM), a value proportional to the expected signal-to-noise ratio of a transmission spectra. π Men c occupies a unique space within escaping atmospheres while possessing a TSM value comparable to JWST targets.

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