TESS Photometry and Radial Velocity Analysis of the sub-Neptune Exoplanet {\pi} Mensae c and the Wider {\pi} Mensae Planetary System
This paper presents a comprehensive analysis of six years of TESS photometry and 22 years of radial velocity data for the Mensae system, yielding significantly improved orbital ephemerides for planets b and c, constraining the mass of a proposed third planet, and identifying Men c as a prime target for future JWST atmospheric studies.