collaborators

7 papers

astro-ph.GA2026

The Galactic Squeeze: How Aggregate and Highly Dynamical Environments Shape Star Formation in the Local Universe

Wesley Van Kempen, Michelle E. Cluver, Edward N. Taylor +2

We investigate how galaxy evolution varies with environment in the nearby Universe by comparing an ``average'' reference volume in the Southern Galactic Pole (SGP) dataset from \ci…

astro-ph.CO2026

Group Therapy for Halos: Advancing Halo Mass Estimation for Galaxy Groups

Welsey Van Kempen, Michelle E. Cluver, Edward N. Taylor +3

Accurate estimation of dark matter halo masses for galaxy groups is central to studies of galaxy evolution and for leveraging group catalogues as cosmological probes. We present a…

astro-ph.GA2025

WALLABY: an untargeted search for H I-bearing ultra-diffuse galaxies uncovers the first known ultra-diffuse galaxy pair

T. O'Beirne, V. A. Kilborn, M. E. Cluver +14

Using the Widefield ASKAP L-band Legacy All-sky Blind surveY (WALLABY) we performed an untargeted search for H I-bearing ultra-diffuse galaxies (UDGs). We identified a core sample…

astro-ph.GA2025

The central spectra of massive star-forming galaxies

Jaimie R. Sheil, Michael J. I . Brown, Virginia A. Kilborn +2

We have examined the nuclear spectra of very massive star-forming galaxies at to understand how they differ from other galaxies with comparable masses, which are typical…

astro-ph.IM2025

Real-Time Active Learning for optimised spectroscopic follow-up: Enhancing early SN Ia classification with the Fink broker

A. Möller, E. E. O. Ishida, J. Peloton +6

Current and future surveys rely on machine learning classification to obtain large and complete samples of transients. Many of these algorithms are restricted by training samples t…

astro-ph.GA2025

MeerKAT view of Hickson Compact Groups: II. HI deficiency in the core and surrounding regions

A. Sorgho, L. Verdes-Montenegro, R. Ianjamasimanana +25

Hickson compact groups (HCGs) offer an ideal environment for investigating galaxy transformation as a result of interactions. It has been established that the evolutionary sequence…