activity
20172021
most citedThe L 98-59 System: Three Transiting, Terrestrial-Sized Planets Orbiting a Nearby M-dwarf

135 citations · 306 across the 6 of their papers we have counts for

collaborators

15 papers

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.EP20211 cited

Significant improvement in planetary system simulations from statistical averaging

David M. Hernandez, Eric Agol, Matthew J. Holman +1

Symplectic integrators are widely used for the study of planetary dynamics and other -body problems. In a study of the outer Solar system, we demonstrate that individual symplec…

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.EP2020108 cited

Predicting the long-term stability of compact multiplanet systems

Daniel Tamayo, Miles Cranmer, Samuel Hadden +11

We combine analytical understanding of resonant dynamics in two-planet systems with machine learning techniques to train a model capable of robustly classifying stability in compac…

astro-ph.EP202016 cited

Modeling Radial Velocity Data of Resonant Planets to Infer Migration Histories

Sam Hadden, Matthew J. Payne

A number of giant planet pairs discovered by the radial velocity method with period ratios may reside in mean motion resonances. Convergent orbital migration and reson…

astro-ph.EP201918 cited

Are long-term -body simulations reliable?

David M. Hernandez, Sam Hadden, Junichiro Makino

-body integrations are used to model a wide range of astrophysical dynamics, but they suffer from errors which make their orbits diverge exponentially in time from the correct o…