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20072026
most citedWSClean: an implementation of a fast, generic wide-field imager for radio astronomy

937 citations · 7.3k across the 150 of their papers we have counts for

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Showing 2016Show all

19 papers · 1 filter

astro-ph.GA2016★ 37 cited

A search for long-timescale, low-frequency radio transients

Tara Murphy, David L. Kaplan, Steve Croft +30

We present a search for transient and highly variable sources at low radio frequencies (150-200 MHz) that explores long timescales of 1-3 years. We conducted this search by compari…

astro-ph.GA2016★ 15 cited

Galactic synchrotron emissivity measurements between 250° < l < 355° from the GLEAM survey with the MWA

H. Su, N. Hurley-Walker, C. A. Jackson +20

Synchrotron emission pervades the Galactic plane at low radio frequencies, originating from cosmic ray electrons interacting with the Galactic magnetic field. Using a low-frequency…

astro-ph.GA2016★ 557 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.CO2016★ 20 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.IM2016★ 170 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.GA2016★ 80 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…