activity
20142017
most citedWSClean: an implementation of a fast, generic wide-field imager for radio astronomy

937 citations · 2.4k across the 17 of their papers we have counts for

collaborators
Showing 2016Show all

6 papers · 1 filter

astro-ph.GA2016557 cited

GaLactic and Extragalactic All-sky Murchison Widefield Array (GLEAM) survey I: A low-frequency extragalactic catalogue

Natasha Hurley-Walker, Joseph R. Callingham, Paul J. Hancock +40

Using the Murchison Widefield Array (MWA), the low-frequency Square Kilometre Array (SKA1 LOW) precursor located in Western Australia, we have completed the GaLactic and Extragalac…

astro-ph.CO201620 cited

Delay Spectrum with Phase-Tracking Arrays: Extracting the HI power spectrum from the Epoch of Reionization

Sourabh Paul, Shiv K. Sethi, Miguel F. Morales +51

The Detection of redshifted 21 cm emission from the epoch of reionization (EoR) is a challenging task owing to strong foregrounds that dominate the signal. In this paper, we propos…

astro-ph.IM2016170 cited

First Season MWA EoR Power Spectrum Results at Redshift 7

A. P. Beardsley, B. J. Hazelton, I. S. Sullivan +63

The Murchison Widefield Array (MWA) has collected hundreds of hours of Epoch of Reionization (EoR) data and now faces the challenge of overcoming foreground and systematic contamin…

astro-ph.GA201680 cited

Low frequency observations of linearly polarized structures in the interstellar medium near the south Galactic pole

Emil Lenc, B. M. Gaensler, X. H. Sun +76

We present deep polarimetric observations at 154 MHz with the Murchison Widefield Array (MWA), covering 625 deg^2 centered on RA=0 h, Dec=-27 deg. The sensitivity available in our…

astro-ph.IM201634 cited

A High Reliability Survey of Discrete Epoch of Reionization Foreground Sources in the MWA EoR0 Field

P. A. Carroll, J. Line, M. F. Morales +61

Detection of the Epoch of Reionization HI signal requires a precise understanding of the intervening galaxies and AGN, both for instrumental calibration and foreground removal. We…

astro-ph.GA201611 cited

The radio spectral energy distribution of infrared-faint radio sources

A. Herzog, R. P. Norris, E. Middelberg +57

Infrared-faint radio sources (IFRS) are a class of radio-loud (RL) active galactic nuclei (AGN) at high redshifts (z > 1.7) that are characterised by their relative infrared faintn…