activity
20242026
collaborators

5 papers

astro-ph.GA2026

A Comprehensive Analysis of WISE Mid-Infrared Colors for Obscured AGN Selection

Anika Goel, Samir Salim, Sara L. Ellison +4

In this paper, we investigate the robustness of WISE mid-IR color selection (W1-W2) for identifying obscured (Type 2) active galactic nuclei (AGNs) at low redshift (z<0.3), using a…

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

Unions with UNIONS: Using galaxy-galaxy lensing to probe galaxy mergers

Isaac Cheng, Jack Elvin-Poole, Michael J. Hudson +12

We use galaxy-galaxy lensing to investigate how the dark matter (DM) haloes and stellar content of galaxies with and $10 \leq \log_{10}(M_\star/\mathrm{M}_…

astro-ph.GA2025

Galaxy evolution in the post-merger regime. III -- The triggering of active galactic nuclei peaks immediately after coalescence

Sara L. Ellison, Leonardo Ferreira, Robert Bickley +6

Galaxy mergers have been shown to trigger AGN in the nearby universe, but the timescale over which this process happens remains unconstrained. The Multi-Model Merger Identifier (MU…

astro-ph.GA2024

Galaxy evolution in the post-merger regime I -- Most merger-induced in-situ stellar mass growth happens post-coalescence

Leonardo Ferreira, Sara L. Ellison, David R. Patton +5

Galaxy mergers can enhance star formation rates throughout the merger sequence, with this effect peaking around the time of coalescence. However, owing to a lack of information abo…