activity
20242026
collaborators

6 papers

astro-ph.EP2026

Quantifying the Contamination of TESS Ecliptic-Plane Light Curves by Minor Planets

Ben Cassese, Justin Vega, Daniel A. Yahalomi +6

Though missions devoted to time series photometry focus primarily on targets far beyond the solar system, their observations can be contaminated by foreground minor planets, especi…

astro-ph.SR2025

ChronoFlow: A Data-Driven Model for Gyrochronology

Phil R. Van-Lane, Joshua S. Speagle, Gwendolyn M. Eadie +6

Gyrochronology is a technique for constraining stellar ages using rotation periods, which change over a star's main sequence lifetime due to magnetic braking. This technique shows…

astro-ph.SR2025

Measuring Long Stellar Rotation Periods (>10 days) from TESS FFI Light Curves is Possible: An Investigation Using TESS and ZTF

Soichiro Hattori, Ruth Angus, Daniel Foreman-Mackey +3

The rotation period of a star is an important quantity that provides insight into its structure and state. For stars with surface features like starspots, their periods can be infe…

astro-ph.SR2025

A Data-Driven M Dwarf Model and Detailed Abundances for 17,000 M Dwarfs in SDSS-V

Aida Behmard, Melissa K. Ness, Andrew R. Casey +6

The cool temperatures of M dwarf atmospheres enable complex molecular chemistry, making robust characterization of M dwarf compositions a long-standing challenge. Recent modificati…

astro-ph.EP2025

Exoplanet Occurrence Rate with Age for FGK Stars in Kepler

Maryum Sayeed, Ruth Angus, Travis Berger +5

We measure exoplanet occurrence rate as a function of isochrone and gyrochronology ages using confirmed and candidate planets identified in Q1-17 DR25 Kepler data. We employ Kepler…

astro-ph.SR2024

zoomies: A tool to infer stellar age from vertical action in Gaia data

Sheila Sagear, Adrian M. Price-Whelan, Sarah Ballard +4

Stellar age measurements are fundamental to understanding a wide range of astronomical processes, including Galactic dynamics, stellar evolution, and planetary system formation. Ho…