collaborators

11 papers

astro-ph.GA2026

Comparison and verification methods to trace interaction-driven disturbances in galaxies

Haotian Lyu, Sarah Brough, Aman Khalid +2

Low surface brightness tidal debris around galaxies, such as tails, streams, and shells, together with other interaction-driven morphological disturbances, serve as valuable indica…

astro-ph.GA2026

Tidal features as tracers of galaxy merger histories: the colours of tidal features in HSC-SSP

A. Desmons, S. Brough, L. Canepa +1

We measure the radial colour profiles of 32,000 galaxies drawn from the Hyper Suprime-Cam Subaru Strategic Program optical imaging survey, including 1415 exhibiting tid…

astro-ph.GA2025

Investigating the imprints of tidal features on simulated galaxy outskirts in LSST-like mock observations

Aman Khalid, Sarah Brough, Garreth Martin +5

Tidal features provide signatures of recent galaxy mergers, offering insights into the role of mergers in galaxy evolution. The Vera C. Rubin Observatory's upcoming Legacy Survey o…

astro-ph.GA2025

Tidal features around simulated groups and cluster galaxies: Enhancement and suppression of merger events through environment in LSST-like mock observations

Aman Khalid, Sarah Brough, Garreth Martin +5

Generally, merger likelihood increases in denser environments; however, the large relative velocities at the centres of dense clusters are expected to reduce the likelihood of merg…

astro-ph.GA2025

Analysing the prevalence of tidal features in HSC-SSP using self-supervised representation learning

A. Desmons, S. Brough, F. Lanusse +2

We use a combination of self-supervised machine learning and visual classification to identify tidal features in a sample of 34,331 galaxies with stellar masses $\log_{10}(M_{*}/\r…

astro-ph.GA2025

Intracluster light is a biased tracer of the dark matter distribution in clusters

J. Butler, G. Martin, N. A. Hatch +3

The diffuse stellar component of galaxy clusters known as intracluster light (ICL) has been proposed as an observable tracer of the cluster's dark matter (DM) halo. Assessing its r…