collaborators

5 papers

astro-ph.EP2026

An Increase in the Galactic Planet Host Fraction Fails to Reproduce the Galactic Height Trend in Planet Occurrence

Christopher Lam, Sarah Ballard, Sheila Sagear +1

While stellar metallicity has long been known to correlate with planetary properties, the galactic metallicity gradient alone does not account for the observed strong trend in plan…

astro-ph.GA2026

The Milky Way's circular velocity curve measured using element abundance gradients

Danny Horta, Adrian M. Price-Whelan, Sergey E. Koposov +4

Spectroscopic surveys now supply precise stellar label measurements such as element abundances for large samples of stars throughout the Milky Way. These element abundances are kno…

astro-ph.GA2025

The dark matter wake of a galactic bar revealed by multichannel Singular Spectral Analysis

Jason A. S. Hunt, Michael S. Petersen, Martin D. Weinberg +7

The Milky Way is known to contain a stellar bar, as are a significant fraction of disc galaxies across the universe. Our understanding of bar evolution, both theoretically and thro…

astro-ph.EP2025

The Orbital Eccentricities of Planets in the Kinematic Thin and Thick Galactic Disks

Sheila Sagear, Sarah Ballard, Kathryne J. Daniel +4

The orbital eccentricity distribution of exoplanets is shaped by a combination of dynamical processes, reflecting both formation conditions and long-term evolution. Probing the orb…

astro-ph.IM2025

PECCARY: A novel approach for characterizing orbital complexity, stochasticity, and regularity

Sóley Ó. Hyman, Kathryne J. Daniel, David A. Schaffner

Permutation Entropy and statistiCal Complexity Analysis for astRophYsics (PECCARY) is a computationally inexpensive, statistical method by which any time-series can be characterize…