activity
19982026
most citedThe 1000 Brightest HIPASS Galaxies: HI Properties

527 citations · 5.7k across the 81 of their papers we have counts for

collaborators

82 papers

astro-ph.GA2026

MUSE-ALMA Haloes XVI: a census of the condensed baryons in z~0.5 HI absorption-selected galaxies

T. O'Beirne, C. Péroux, M. Zwaan +16

We use the MUSE-ALMA Haloes sample to build a census of the condensed baryons (stars and cold gas) to study the multiphase interstellar medium and circumgalactic medium (CGM). The…

astro-ph.GA2026

The Bright Future of the Dark and Dim Universe

N. Deg, Alejandro Benitez-Llambay, Elizabeth A. K. Adams +5

This chapter investigates the low-mass frontier of galaxy formation through two complementary populations: the starless Reionization-Limited HI Clouds (RELHICs) that trace the ``da…

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★ 1 cited

WALLABY Pilot Survey: A gas-rich diffuse dwarf on the baryonic Tully Fisher relation

Rebecca Dudley, N. Deg, Kristine Spekkens +5

Diffuse dwarf galaxies, and particularly ultra diffuse galaxies (UDGs), challenge our understanding of galaxy formation and the role of dark matter due to their large sizes, low su…

astro-ph.GA2025

WALLABY Pilot Survey: Characterizing Low Rotation Kinematically Modelled Galaxies

N. Deg, K. Spekkens, N. Arora +20

Many of the tensions in cosmological models of the Universe lie in the low mass, low velocity regime. Probing this regime requires a statistically significant sample of galaxies wi…

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…