activity
20242026
collaborators

6 papers

astro-ph.HE2026

Merger Driven or Internal Evolution? A New Morphological Study of Tidal Disruption Event Host Galaxies

Janet N. Y. Chang, Connor Bottrell, Lixin Dai +7

The host galaxies of tidal disruption events (TDEs) show enhanced central stellar concentration and are preferentially found in poststarburst and green valley populations. This con…

astro-ph.GA2026

Galaxy Mergers in UNIONS -- II: Predicting Timescales in the Post-Merger Regime

Leonardo Ferreira, Sara L. Ellison, David R. Patton +3

Galaxy mergers are critical events that influence galaxy evolution by driving processes such as enhanced star formation, quenching, and active galactic nucleus (AGN) activity. Howe…

astro-ph.GA2025

Interacting galaxies in the IllustrisTNG simulations - IX: Mini mergers trigger AGN in cosmological simulations

Shoshannah Byrne-Mamahit, Sara L. Ellison, David R. Patton +3

Galaxy mergers are transformative events that can cause gaseous inflows capable of triggering active galactic nuclei (AGN). Previous studies of AGN in simulations have mainly focus…

astro-ph.GA2025

Low redshift post-starburst galaxies host abundant HI reservoirs

Sara L. Ellison, Qifeng Huang, Dong Yang +8

Studying the gas content of post-starburst (PSB) galaxies can provide valuable clues regarding the process of fast quenching. Although previous works have studied the molecular gas…

astro-ph.GA2025

UNIONS: The Ultraviolet Near-Infrared Optical Northern Survey

Stephen Gwyn, Alan W. McConnachie, Jean-Charles Cuillandre +86

The Ultraviolet Near-Infrared Optical Northern Survey (UNIONS) is a "collaboration of collaborations" that is using the Canada-France-Hawai'i Telescope, the Pan-STARRS telescopes,…

astro-ph.GA2024

Galaxy evolution in the post-merger regime. II -- Post-merger quenching peaks within 500 Myr of coalescence

Sara L. Ellison, Leonardo Ferreira, Vivienne Wild +3

(Abridged) Mechanisms for quenching star formation in galaxies remain hotly debated, with galaxy mergers an oft-proposed pathway. In Ellison et al. (2022) we tested this scenario b…