activity
20122026
most citedCALIFA, the Calar Alto Legacy Integral Field Area survey: IV. Third Public data release

272 citations · 2.1k across the 54 of their papers we have counts for

collaborators

54 papers

astro-ph.GA2026

Resolved HI and Environmental Dynamics

M. Ramatsoku, P. Serra, N. Deg +8

Spatially resolved, deep HI observations from SKA precursors and pathfinders such as MeerKAT, FAST, and ASKAP have demonstrated their ability to reveal the complex interactions bet…

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

WALLABY Pilot Survey: the extensive interaction of NGC 4532 and DDO 137 with the Virgo cluster

L. Staveley-Smith, K. Bekki, A. Boselli +16

As part of the pilot survey of the Widefield ASKAP L-band Legacy All-sky Survey (WALLABY), high-resolution neutral atomic hydrogen (HI) observations of the dwarf galaxy pair NGC 45…

astro-ph.GA2025★ 12 cited

HI within and around observed and simulated galaxy discs -- Comparing MeerKAT observations with mock data from TNG50 and FIRE-2

A. Marasco, W. J. G. de Blok, F. M. Maccagni +12

Atomic hydrogen (HI) is an ideal tracer of gas flows in and around galaxies, and it is uniquely observable in the nearby Universe. Here we make use of wide-field (~1 square degree)…

astro-ph.GA2025★ 1 cited

WALLABY Pilot Survey & ASymba: Comparing HI Detection Asymmetries to the SIMBA Simulation

Mathieu Perron-Cormier, Nathan Deg, Kristine Spekkens +15

An avenue for understanding cosmological galaxy formation is to compare morphometric parameters in observations and simulations of galaxy assembly. In this second paper of the ASym…

astro-ph.GA2024★ 2 cited

MIGHTEE-HI: The star-forming properties of HI selected galaxies

Madalina N. Tudorache, M. J. Jarvis, A. A. Ponomareva +9

The interplay between atomic gas, the star-formation history of a galaxy and its environment are intrinsically linked, and we need to decouple these dependencies to understand thei…

astro-ph.GA2024★ 9 cited

Searching for HI around MHONGOOSE Galaxies via Spectral Stacking

S. Veronese, W. J. G. de Blok, J. Healy +19

The observed star formation rates of galaxies in the Local Universe suggests that they are replenishing their gas reservoir across cosmic time. Cosmological simulations predict tha…

astro-ph.GA2024★ 7 cited

WALLABY Pilot Survey: Gas-Rich Galaxy Scaling Relations from Marginally-Resolved Kinematic Models

N. Deg, N. Arora, K. Spekkens +21

We present the first set of galaxy scaling relations derived from kinematic models of the Widefield ASKAP L-band Legacy All-sky Blind surveY (WALLABY) pilot phase observations. Com…

astro-ph.GA2024★ 2 cited

WALLABY Pilot Survey: Star Formation Enhancement and Suppression in Gas-rich Galaxy Pairs

Qifeng Huang, Jing Wang, Xuchen Lin +16

Galaxy interactions can significantly affect the star formation in galaxies, but it remains a challenge to achieve a consensus on the star formation rate (SFR) enhancement in galax…

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★ 13 cited

MHONGOOSE discovery of a gas-rich low-surface brightness galaxy in the Dorado Group

F. M. Maccagni, W. J. G. de Blok, P. E. Mancera Piña +28

We present the discovery of a low-mass gas-rich low-surface brightness galaxy in the Dorado Group, at a distance of 17.7 Mpc. Combining deep MeerKAT 21-cm observations from the Mee…

astro-ph.GA2024★ 46 cited

MHONGOOSE -- A MeerKAT Nearby Galaxy HI Survey

W. J. G. de Blok, J. Healy, F. M. Maccagni +57

The MHONGOOSE (MeerKAT HI Observations of Nearby Galactic Objects: Observing Southern Emitters) survey maps the distribution and kinematics of the neutral atomic hydrogen (HI) gas…

astro-ph.GA2024★ 13 cited

Possible origins of anomalous HI gas around MHONGOOSE galaxy, NGC 5068

J. Healy, W. J. G. de Blok, F. M. Maccagni +17

The existing reservoirs of neutral atomic hydrogen gas (HI) in galaxies are insufficient to have maintained the observed levels of star formation without some kind of replenish…

astro-ph.GA2024

WALLABY Pilot Survey: An 'Almost' Dark Cloud near the Hydra Cluster

T. O'Beirne, L. Staveley-Smith, O. I. Wong +20

We explore the properties of an 'almost' dark cloud of neutral hydrogen (HI) using data from the Widefield ASKAP L-band Legacy All-sky Survey (WALLABY). Until recently, WALLABY J10…

astro-ph.GA2023

WALLABY Pre-Pilot Survey: Ultra-Diffuse Galaxies in the Eridanus Supergroup

B. -Q. For, K. Spekkens, L. Staveley-Smith +12

We present a pilot study of the atomic neutral hydrogen gas (HI) content of ultra-diffuse galaxy (UDG) candidates. In this paper, we use the pre-pilot Eridanus field data from the…

astro-ph.GA2023★ 25 cited

WALLABY Pilot Survey: the Potential Polar Ring Galaxies NGC~4632 and NGC~6156

N. Deg, R. Palleske, K. Spekkens +24

We report on the discovery of two potential polar ring galaxies (PRGs) in the WALLABY Pilot Data Release 1 (PDR1). These untargetted detections, cross-matched to NGC 4632 and NGC 6…

astro-ph.GA2023★ 7 cited

WALLABY Pilot Survey: The diversity of HI structural parameters in nearby galaxies

T. N. Reynolds, B. Catinella, L. Cortese +22

We investigate the diversity in the sizes and average surface densities of the neutral atomic hydrogen (HI) gas discs in ~280 nearby galaxies detected by the Widefield ASKAP L-band…

astro-ph.GA2023★ 6 cited

Measuring Galaxy Asymmetries in 3D

N. Deg, M. Perron-Cormier, K. Spekkens +3

One of the commonly used non-parametric morphometric statistics for galaxy profiles and images is the asymmetry statistic. With an eye to current and upcoming large neutral hydroge…

astro-ph.GA2023★ 25 cited

MIGHTEE-HI: The first MeerKAT HI mass function from an untargeted interferometric survey

Anastasia A. Ponomareva, Matt J. Jarvis, Hengxing Pan +17

We present the first measurement of the HI mass function (HIMF) using data from MeerKAT, based on 276 direct detections from the MIGHTEE Survey Early Science data covering a period…

astro-ph.GA2023★ 7 cited

WALLABY Pilot Survey: Hydra Cluster Galaxies UV and HI morphometrics

Benne W. Holwerda, Frank Bigiel, Albert Bosma +16

Galaxy morphology in atomic hydrogen (HI) and in the ultra-violet (UV) are closely linked. This has motivated their combined use to quantify morphology over the full H i disk for b…

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…