activity
19982018
most citedThe 1000 Brightest HIPASS Galaxies: HI Properties

527 citations · 3.2k across the 41 of their papers we have counts for

collaborators

41 papers

astro-ph.GA2018★ 13 cited

The Neutral Hydrogen Properties of Galaxies in Gas-rich Groups

Robert Džudžar, Virginia Kilborn, Gerhardt Meurer +23

We present an analysis of the integrated neutral hydrogen (HI) properties for 27 galaxies within nine low mass, gas-rich, late-type dominated groups which we denote "Choirs". We fi…

astro-ph.GA2018★ 9 cited

Near-identical star formation rate densities from H and FUV at redshift zero

Fiona M. Audcent-Ross, Gerhardt R. Meurer, O. I. Wong +27

For the first time both H and far-ultraviolet (FUV) observations from an HI-selected sample are used to determine the dust-corrected star formation rate density (SFRD: )…

astro-ph.CO2013★ 13 cited

Tidal Tails of Minor Mergers II: Comparing Star Formation in the Tidal Tails of NGC 2782

Karen Knierman, Paul Scowen, Todd Veach +5

The peculiar spiral NGC 2782 is the result of a minor merger with a mass ratio ~4:1 occurring ~200 Myr ago. This merger produced a molecular and HI rich, optically bright Eastern t…

astro-ph.CO2013★ 10 cited

Choirs, HI Galaxy Groups: Catalogue and Detection of Star-forming Dwarf Group Members

Sarah M. Sweet, Gerhardt Meurer, Michael J. Drinkwater +24

Hα observations centred on galaxies selected from the HI Parkes All Sky Survey (HIPASS, Barnes et al. 2001) typically show one and sometimes two star-forming galaxies within the ap…

astro-ph.CO2012★ 73 cited

The Infrared Light Curve of SN 2011fe in M101 and the Distance to M101

T. Matheson, R. R. Joyce, L. E. Allen +42

We present near infra-red light curves of supernova (SN) 2011fe in M101, including 34 epochs in H band starting fourteen days before maximum brightness in the B-band. The light cur…

astro-ph.CO2012★ 16 cited

Tidal Tails of Minor Mergers: Star Formation Efficiency in the Western Tail of NGC 2782

Karen Knierman, Patricia Knezek, Paul Scowen +2

While major mergers and their tidal debris are well studied, they are less common than minor mergers (mass ratios < 0.3). The peculiar spiral NGC 2782 is the result of a merger bet…