activity
20152021
most citedHybrid Symplectic Integrators for Planetary Dynamics

146 citations · 385 across the 8 of their papers we have counts for

collaborators

21 papers

astro-ph.EP20211 cited

A Criterion for the Onset of Chaos in Compact, Eccentric Multiplanet Systems

Daniel Tamayo, Norman Murray, Scott Tremaine +1

We derive a semi-analytic criterion for the presence of chaos in compact, eccentric multiplanet systems. Beyond a minimum semimajor-axis separation, below which the dynamics are ch…

astro-ph.SR20211 cited

TIC 454140642: A Compact, Coplanar, Quadruple-lined Quadruple Star System Consisting of Two Eclipsing Binaries

Veselin B. Kostov, Brian P. Powell, Guillermo Torres +30

We report the discovery of a compact, coplanar, quadruply-lined, eclipsing quadruple star system from TESS data, TIC 454140642, also known as TYC 0074-01254-1. The target was first…

astro-ph.EP2021

How Close are Compact Multi-Planet Systems to the Stability Limit?

Samuel W. Yee, Daniel Tamayo, Samuel Hadden +1

Transit surveys have revealed a significant population of compact multi-planet systems, containing several sub-Neptune-mass planets on close-in, tightly-packed orbits. These system…

astro-ph.EP2021

A Bayesian neural network predicts the dissolution of compact planetary systems

Miles Cranmer, Daniel Tamayo, Hanno Rein +5

Despite over three hundred years of effort, no solutions exist for predicting when a general planetary configuration will become unstable. We introduce a deep learning architecture…

astro-ph.EP2020

Revisiting the Architecture of the KOI-89 System

Kento Masuda, Daniel Tamayo

While high stellar obliquities observed in exoplanetary systems may be attributed to processes that tilt the planetary orbits, it is also possible that they reflect misalignments b…

astro-ph.EP2020

Stability Constrained Characterization of Multiplanet Systems

Daniel Tamayo, Christian Gilbertson, Daniel Foreman-Mackey

Many discovered multiplanet systems are tightly packed. This implies that wide parameter ranges in masses and orbital elements can be dynamically unstable and ruled out. We present…