activity
20202025
most citedWALLABY Pilot Survey: Public release of HI data for almost 600 galaxies from phase 1 of ASKAP pilot observations

47 citations · 123 across the 12 of their papers we have counts for

collaborators

12 papers

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

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★ 1 cited

The Polarisation Sky Survey of the Universe's Magnetism (POSSUM): Science Goals and Survey Description

B. M. Gaensler, G. H. Heald, N. M. McClure-Griffiths +57

The Australian SKA Pathfinder (ASKAP) offers powerful new capabilities for studying the polarised and magnetised Universe at radio wavelengths. In this paper, we introduce the Pola…

astro-ph.GA2025

WALLABY pilot survey: properties of HI-selected dark sources and low surface brightness galaxies

T. O'Beirne, L. Staveley-Smith, V. A. Kilborn +13

We examine the optical counterparts of the 1829 neutral hydrogen (HI) detections in three pilot fields in the Widefield ASKAP L-band Legacy All-sky Blind surveY (WALLABY) using dat…

astro-ph.GA2024★ 2 cited

WALLABY Pilot Survey: Public data release of ~1800 HI sources and high-resolution cut-outs from Pilot Survey Phase 2

C. Murugeshan, N. Deg, T. Westmeier +20

We present the Pilot Survey Phase 2 data release for the Wide-field ASKAP L-band Legacy All-sky Blind surveY (WALLABY), carried-out using the Australian SKA Pathfinder (ASKAP). We…

astro-ph.GA2024

WALLABY Pilot Survey: the Tully-Fisher relation in the NGC 4808, Vela and NGC 5044 fields

Jeremy Mould, T. H. Jarrett, Hélène Courtois +18

The Tully-Fisher Relation (TFR) is a well-known empirical relationship between the luminosity of a spiral galaxy and its circular velocity, allowing us to estimate redshift indepen…

astro-ph.GA2023★ 26 cited

WALLABY Pilot Survey: HI in the host galaxy of a Fast Radio Burst

M. Glowacki, K. Lee-Waddell, A. T. Deller +17

We report on the commensal ASKAP detection of a fast radio burst (FRB), FRB20211127I, and the detection of neutral hydrogen (HI) emission in the FRB host galaxy, WALLABYJ131913-185…

astro-ph.IM2023

Asymmetric distribution of data products from WALLABY, an SKA precursor neutral hydrogen survey

Manuel Parra-Royon, Austin Shen, Tristan Reynolds +6

The Widefield ASKAP L-band Legacy All-sky Blind surveY (WALLABY) is a neutral hydrogen survey (HI) that is running on the Australian SKA Pathfinder (ASKAP), a precursor telescope f…

astro-ph.IM2023★ 22 cited

SKA Science Data Challenge 2: analysis and results

P. Hartley, A. Bonaldi, R. Braun +105

The Square Kilometre Array Observatory (SKAO) will explore the radio sky to new depths in order to conduct transformational science. SKAO data products made available to astronomer…

astro-ph.GA2022★ 22 cited

WALLABY Pilot Survey: Public release of HI kinematic models for more than 100 galaxies from phase 1 of ASKAP pilot observations

N. Deg, K. Spekkens, T. Westmeier +29

We present the Widefield ASKAP L-band Legacy All-sky Blind surveY (WALLABY) Pilot Phase I HI kinematic models. This first data release consists of HI observations of three fields i…

astro-ph.GA2022★ 47 cited

WALLABY Pilot Survey: Public release of HI data for almost 600 galaxies from phase 1 of ASKAP pilot observations

T. Westmeier, N. Deg, K. Spekkens +49

We present WALLABY pilot data release 1, the first public release of HI pilot survey data from the Wide-field ASKAP L-band Legacy All-sky Blind Survey (WALLABY) on the Australian S…

astro-ph.GA2020★ 3 cited

A new way to constrain the densities of intra-group medium in groups of galaxies with convolutional neural networks

Austin X. Shen, Kenji Bekki

Ram pressure (RP) can influence the evolution of cold gas content and star formation rates of galaxies. One of the key parameters for the strength of RP is the density of intra-gro…