activity
20162021
most citedCalibration and Stokes Imaging with Full Embedded Element Primary Beam Model for the Murchison Widefield Array

64 citations · 207 across the 8 of their papers we have counts for

collaborators

9 papers

astro-ph.CO20212 cited

Epoch of Reionization Power Spectrum Limits from Murchison Widefield Array Data Targeted at EoR1 Field

M. Rahimi, B. Pindor, J. L. B. Line +28

Current attempts to measure the 21cm Power Spectrum of neutral hydrogen during the Epoch of Reionization are limited by systematics which produce measured upper limits above both t…

astro-ph.CO20217 cited

Constraining the 21cm brightness temperature of the IGM at =6.6 around LAEs with the Murchison Widefield Array

Cathryn M. Trott, C. H. Jordan, J. L. B. Line +29

The locations of Ly- emitting galaxies (LAEs) at the end of the Epoch of Reionisation (EoR) are expected to correlate with regions of ionised hydrogen, traced by the redshifted…

astro-ph.GA20217 cited

The GLEAM 200 MHz Local Radio Luminosity Function for AGN and Star-forming Galaxies

T. M. O. Franzen, N. Seymour, E. M. Sadler +24

The GaLactic and Extragalactic All-sky Murchison Widefield Array (GLEAM) is a radio continuum survey at 76-227 MHz of the entire southern sky (Declination ) with an angular…

astro-ph.GA2018

Galactic synchrotron distribution derived from 152 HII region absorption features in the full GLEAM survey

H. Su, J. P. Macquart, N. Hurley-Walker +22

We derive the synchrotron distribution in the Milky Way disk from HII region absorption observations over -40° < l < 40° at six frequencies of 76.2, 83.8, 91.5, 99.2, 106.9, and 11…

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…