activity
20092026
most citedThe Australia Telescope 20 GHz Survey: The Source Catalogue

357 citations · 919 across the 35 of their papers we have counts for

collaborators
Showing 2018Show all

5 papers · 1 filter

astro-ph.GA2018★ 10 cited

Interplanetary Scintillation studies with the Murchison Wide-field Array IV: The hosts of sub-arcsecond compact sources at low radio frequencies

Elaine M. Sadler, Rajan Chhetri, John Morgan +3

Around 10% of bright low-frequency radio sources observed with the Murchison Widefield Array (MWA) show strong Interplanetary Scintillation (IPS) on timescales of a few seconds, im…

astro-ph.GA2018★ 12 cited

The Murchison Widefield Array Transients Survey (MWATS). A search for low frequency variability in a bright Southern hemisphere sample

M. E. Bell, Tara Murphy, P. J. Hancock +38

We report on a search for low-frequency radio variability in 944 bright (> 4Jy at 154 MHz) unresolved, extragalactic radio sources monitored monthly for several years with the Murc…

astro-ph.GA2018★ 2 cited

The MWA GLEAM 4-Jy (G4Jy) Sample

Sarah V. White, Thomas M. O. Franzen, O. Ivy Wong +15

Powerful radio-galaxies feature heavily in our understanding of galaxy evolution. However, when it comes to studying their properties as a function of redshift and/or environment,…

astro-ph.GA2018★ 19 cited

Interplanetary Scintillation with the Murchison Widefield Array V: An All-sky Survey of Compact Sources using a Modern Low-frequency Radio Telescope

J. S. Morgan, J-P. Macquart, R. Chhetri +3

We describe the parameters of a low-frequency all-sky survey of compact radio sources using Interplanetary Scintillation (IPS), undertaken with the Murchison Widefield Array (MWA).…

astro-ph.GA2018★ 11 cited

Interplanetary Scintillation studies with the Murchison Wide-field Array III: Comparison of source counts and densities for radio sources and their sub-arcsecond components at 162 MHz

R. Chhetri, R. D. Ekers, J. Morgan +2

We use Murchison Widefield Array observations of interplanetary scintillation (IPS) to determine the source counts of point (0.3 arcsecond extent) sources and of all sources wit…