The true masses of radial-velocity exoplanets constrained by stability
astro-ph.EP, astro-ph.IM
Submitted: 2026-08-27
Updated: 2026-08-27
Code: https://github.com/xbyrne/cinemas
Terminology
Sources
- The Barnard's Star Planetary System: Stability, Composition, and Evolution of Four Sub-Earth Exoplanets
- The NEID Earth Twin Survey. IV. Confirming an 89 d, $m\sin i=10~\mathrm{M_\oplus}$ Planet Orbiting a Nearby Sun-like Star
- Frequency of planets orbiting M dwarfs in the Solar neighbourhood
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