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20172026
most citedWALLABY pilot survey: Spatially resolved gas scaling relations within the stellar discs of nearby galaxies

8 citations · 20 across the 10 of their papers we have counts for

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9 papers · 1 filter

astro-ph.GA2026

Bridging the mass gap: Diffuse radio emission in GAMA galaxy groups using EMU and DINGO survey data

Sai Wagh, Tessa Vernstrom, Luke J. M. Davies +11

Diffuse radio emission provides a powerful probe of non-thermal processes in the large-scale structure, yet its properties in galaxy groups remain poorly constrained. Using deep 94…

astro-ph.GA2026

DINGO/GAMA /WAVES: HI-halo mass relation

Ajay Dev, Martin Meyer, Simon P. Driver +17

We investigate the relation between neutral atomic hydrogen (HI) and dark matter halo mass (HIHM) using observations from the Deep Investigation of Neutral Gas Origins (DINGO) pilo…

astro-ph.GA2026

WALLABY pilot survey: HI depletion times within the stellar discs of nearby galaxies

Seona Lee, Barbara Catinella, Tobias Westmeier +12

Neutral atomic hydrogen (HI) reservoirs typically extend far beyond the inner star-forming regions of galaxies, and global HI measurements, which mix these distinct environments, l…

astro-ph.GA20258 cited

WALLABY pilot survey: Spatially resolved gas scaling relations within the stellar discs of nearby galaxies

Seona Lee, Barbara Catinella, Tobias Westmeier +13

The scatter in global atomic hydrogen (HI) scaling relations is partly attributed to differences in how HI and stellar properties are measured, with HI reservoirs typically extendi…

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.GA2025

WALLABY Pilot Survey: kNN identification of perturbed galaxies through HI morphometrics

B. W. Holwerda, Helga Dénes, J. Rhee +11

Galaxy morphology in stellar light can be described by a series of "non-parametric" or "morphometric" parameters, such as concentration-asymmetry-smoothness, Gini, , and Se…