activity
19962023
most citedDust Absorption And The Ultraviolet Luminosity Density At z \approx 3 As Calibrated By Local Starburst Galaxies

1.1k citations · 10k across the 123 of their papers we have counts for

collaborators

123 papers

astro-ph.GA2023★ 1 cited

On the origin of the anomalous gas, non-declining rotation curve and disc asymmetries in NGC253

Xuanyi Lyu, T. Westmeier, Gerhardt R. Meurer +1

We present a multi-wavelength (from far ultraviolet to HI emission) study of star formation feedback on the kinematics of the interstellar medium in the Sculptor Galaxy, NGC253. It…

astro-ph.GA2022★ 9 cited

WALLABY Pilot Survey: HI gas kinematics of galaxy pairs in cluster environment

Shin-Jeong Kim, Se-Heon Oh, Jing Wang +22

We examine the HI gas kinematics of galaxy pairs in two clusters and a group using Australian Square Kilometre Array Pathfinder (ASKAP) WALLABY pilot survey observations. We compar…

astro-ph.GA2022★ 17 cited

WALLABY Pre-Pilot and Pilot Survey: the Tully Fisher Relation in Eridanus, Hydra, Norma and NGC4636 fields

Hélène M. Courtois, Khaled Said, Jeremy Mould +28

The WALLABY pilot survey has been conducted using the Australian SKA Pathfinder (ASKAP). The integrated 21-cm HI line spectra are formed in a very different manner compared to usua…

astro-ph.GA2022★ 12 cited

LADUMA: Discovery of a luminous OH megamaser at

Marcin Glowacki, Jordan D. Collier, Amir Kazemi-Moridani +65

In the local Universe, OH megamasers (OHMs) are detected almost exclusively in infrared-luminous galaxies, with a prevalence that increases with IR luminosity, suggesting that they…

astro-ph.HE2021★ 4 cited

Physics of radio emission in the long-period pulsars

P B Jones

Recent multi-frequency measurements of pulse widths W50 for the long-period pulsar J0250+5854 by Agar et al provide a unique insight to the emission process owing to its small pola…

astro-ph.GA2020★ 4 cited

Environmental processing of galaxies in HI-rich groups

Robert Džudžar, Virginia Kilborn, Sarah M. Sweet +3

We present and explore the resolved atomic hydrogen (HI) content of 13 HI-rich and late-type dominated groups denoted `Choirs'. We quantify the HI content of the Choir galaxies wit…