activity
20152017
most citedCalibration and Stokes Imaging with Full Embedded Element Primary Beam Model for the Murchison Widefield Array

64 citations · 432 across the 12 of their papers we have counts for

collaborators

10 papers

astro-ph.GA201725 cited

The SAMI Galaxy Survey: The Low-Redshift Stellar Mass Tully-Fisher Relation

J. V. Bloom, S. M. Croom, J. J. Bryant +22

We investigate the Tully-Fisher Relation (TFR) for a morphologically and kine- matically diverse sample of galaxies from the SAMI Galaxy Survey using 2 dimensional spatially resolv…

astro-ph.HE201744 cited

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

R. Chhetri, J. Morgan, R. D. Ekers +5

We report the first astrophysical application of the technique of wide-field Interplanetary Scintillation (IPS) with the Murchison Widefield Array (MWA). This powerful technique al…

astro-ph.IM201764 cited

Calibration and Stokes Imaging with Full Embedded Element Primary Beam Model for the Murchison Widefield Array

M. Sokolowski, T. Colegate, A. T. Sutinjo +22

The Murchison Widefield Array (MWA), located in Western Australia, is one of the low-frequency precursors of the international Square Kilometre Array (SKA) project. In addition to…

astro-ph.GA201757 cited

The Spectral Energy Distribution of Powerful Starburst Galaxies I: Modelling the Radio Continuum

T J Galvin, N Seymour, J Marvil +24

We have acquired radio continuum data between 70\,MHz and 48\,GHz for a sample of 19 southern starburst galaxies at moderate redshifts () with the aim of separat…

astro-ph.IM201730 cited

A high resolution foreground model for the MWA EoR1 field: model and implications for EoR power spectrum analysis

P. Procopio, R. B. Wayth, J. Line +23

The current generation of experiments aiming to detect the neutral hydrogen signal from the Epoch of Reionisation (EoR) is likely to be limited by systematic effects associated wit…

astro-ph.GA201726 cited

Connecting X-ray absorption and 21cm neutral hydrogen absorption in obscured radio AGN

V. A. Moss, J. R. Allison, E. M. Sadler +22

Many radio galaxies show the presence of dense and dusty gas near the active nucleus. This can be traced by both 21cm HI absorption and soft X-ray absorption, offering new insight…