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most citedThe Astrometric Resoeccentric Degeneracy: Eccentric Single Planets Mimic 2:1 Resonant Planet Pairs in Astrometry

3 citations · 11 across the 18 of their papers we have counts for

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astro-ph.EP2025

Constraining the Occurrence of ZLK-Induced White Dwarf Pollution with Dissipative Precession

Isabella Trierweiler, Konstantin Gerbig, Malena Rice

Von Zeipel-Lidov-Kozai (ZLK) oscillations, induced by bound, perturbative companions to white dwarfs, have been suggested as a dynamical mechanism that may contribute to white dwar…

astro-ph.EP2025★ 3 cited

The Astrometric Resoeccentric Degeneracy: Eccentric Single Planets Mimic 2:1 Resonant Planet Pairs in Astrometry

Daniel A. Yahalomi, Tiger Lu, Philip J. Armitage +4

Detections of long-period giant exoplanets will expand dramatically with Gaia Data Release 4 (DR4), but interpreting these signals will require care. We derive the astrometric reso…

astro-ph.EP2025★ 2 cited

A High-Precision, Differentiable Code for Solar System Ephemerides

Ben Cassese, Malena Rice, Tiger Lu

We present jorbit, a python/JAX library designed to enable modern data-driven numerical studies of the solar system. Written entirely in JAX, an auto-differentiable and optionally…

astro-ph.EP2025★ 2 cited

Do White Dwarfs Sample Water-Rich Planetary Material?

Isabella L. Trierweiler, Carl Melis, Érika Le Bourdais +9

Polluted white dwarfs offer a unique way to directly probe the compositions of exoplanetary bodies. We examine the water content of accreted material using the oxygen abundances of…

astro-ph.EP2025★ 2 cited

The Formation of Double Hot Jupiter Systems through von Zeipel-Lidov-Kozai Migration

Yurou Liu, Tiger Lu, Malena Rice

The von Zeipel-Lidov-Kozai (ZLK) mechanism with tidal friction has been demonstrated as a promising avenue to generate hot Jupiters in stellar binary systems. Previous population s…

astro-ph.EP2025

JWST Coronagraphic Images of 14 Her c: a Cold Giant Planet in a Dynamically Hot, Multi-planet System

Daniella C. Bardalez Gagliuffi, William O. Balmer, Laurent Pueyo +16

Most observed multi-planet systems are coplanar, in a dynamically "cold" configuration of concentric orbits like our own Solar System. With the James Webb Space Telescope (JWST) we…

astro-ph.EP2025

Peekaboo: Secular Resonances from Evolving Stellar Oblateness Impede Transit Detection

Thea Faridani, Smadar Naoz, Gongjie Li +2

Secular resonances in exoplanet systems occur when two or more planets have commensurabilities in the precession rates of their orbital elements, causing an exchange of angular mom…

astro-ph.EP2025

Collisional Fragmentation Support in TRACE

Tiger Lu, Haniyeh Tajer, David M. Hernandez +3

We present improved collision support for TRACE, a state-of-the-art hybrid integrator in REBOUND. TRACE now supports collisional fragmentation and can handle both removing and addi…

astro-ph.EP2025

The Case for Edge-On Binaries: An Avenue Toward Comparative Exoplanet Demographics

Joseph E. Hand, Malena Rice, Konstantin Gerbig

Most Sun-like and higher-mass stars reside in systems that include one or more gravitationally bound stellar companions. These systems offer an important probe of planet formation…