3 citations · 10 across the 9 of their papers we have counts for
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astro-ph.EP2025★ 3 cited
Close-in compact super-Earth systems emerging from resonant chains: slow destabilization by unseen remnants of formation
Max Goldberg, Antoine C. Petit
Planet formation simulations consistently predict compact systems of numerous small planets in chains of mean motion resonances formed by planet-disk interaction, but transiting pl…
astro-ph.EP2025★ 2 cited
The Dynamical History of the Kepler-221 Planet System
Tian Yi, Chris W. Ormel, Shuo Huang +1
Kepler-221 is a G-type star hosting four planets. In this system, planets b, c, and e are in (or near) a 6:3:1 three-body resonance even though the planets' period ratios show sign…
astro-ph.EP2025
From Stability to Instability: Characterizing the Eccentricities of Multi-planet Systems in the California Kepler Survey as a Means of Studying Stability
Matthew J. Doty, Lauren M. Weiss, Matthias Y. He +1
Understanding the stability of exoplanet systems is crucial for constraining planetary formation and evolution theories. We use the machine-learning stability indicator, SPOCK, to…