collaborators

7 papers

astro-ph.GA2026

Automated Computer Vision Cluster Identification in the Fireworks Galaxy

Debby Tran, Benjamin F. Williams, Emily M. Levesque +5

The paper describes a computer‑vision method that uses Hubble Space Telescope UV images to automatically detect and measure young star cluster candidates in the Fireworks Galaxy (N…

astro-ph.GA2026

A Multiwavelength Inventory for the Local Group L-band Survey I: Atlas and Radial Profiles of Local Group Galaxies

Cosima Eibensteiner, Adam K. Leroy, Jiayi Sun +21

Resolving atomic gas at pc physical resolution is currently feasible only for the very nearest galaxies. We combine 120 pc resolution HI data using the Karl G. Jansky…

astro-ph.SR2026

Searching for Stellar Activity Cycles using Flares II: The TESS CVZ

Tobin M. Wainer, Holland M. Stuart, Guadalupe Tovar Mendoza +3

The paper analyzes seven years of TESS short‑cadence data for over 14,000 stars in the Continuous Viewing Zone to detect long‑term changes in flare activity, identifying 17 stars w…

astro-ph.HE2026

Optical Counterparts to X-ray sources in LSST DP1

Yuankun, Wang, Eric C. Bellm +9

The paper crossmatches a combined X‑ray source catalog with the Vera C. Rubin Observatory LSST Data Preview 1 to identify optical counterparts across six fields, reporting 2314 mat…

astro-ph.GA2026

The Panchromatic Hubble Andromeda Southern Treasury (PHAST). II. The Spatially Resolved Recent Star Formation History in M31

Tobin M. Wainer, Benjamin F. Williams, Zhuo Chen +19

We use Hubble Space Telescope optical imaging from the Panchromatic Hubble Andromeda Southern Treasury (PHAST) to measure the spatially resolved recent star formation history (SFH)…

astro-ph.SR2026

The Timescales of Embedded Star Formation as Observed in STARFORGE

Tobin M. Wainer, Julianne J. Dalcanton, Michael Y. Grudić +7

Star formation occurs within dusty molecular clouds that are then disrupted by stellar feedback. However, the timing and physical mechanisms that govern the transition from deeply…