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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 1.

The process of deducing transit-midpoint priors from π Men c TESS photometry data. The x-axis is listed in units of TESS Barycentric Julian Date (BTJD), which is equal to BJD – 2457000. Top: TESS sector 13. The dark gray points are binned and light gray unbinned. All binned data points the pipeline flags as being part of a transit (Z ≤ −3.3 in this case) are highlighted in red. Bottom: a singular transit. The transit-midpoint initial guess is the median of the red points. This process allows for an automatic and streamlined selection of transit-midpoint priors.

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