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20032017
most citedWSClean: an implementation of a fast, generic wide-field imager for radio astronomy

937 citations · 2.3k across the 19 of their papers we have counts for

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7 papers · 1 filter

astro-ph.IM2016★ 37 cited

PUMA: The Positional Update and Matching Algorithm

J. L. B. Line, R. L. Webster, B. Pindor +2

We present new software to cross-match low-frequency radio catalogues: the Positional Update and Matching Algorithm (PUMA). PUMA combines a positional Bayesian probabilistic approa…

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.IM2016★ 34 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.IM2015★ 61 cited

The High Time and Frequency Resolution Capabilities of the Murchison Widefield Array

S. E. Tremblay, S. M. Ord, N. D. R. Bhat +37

The science cases for incorporating high time resolution capabilities into modern radio telescopes are as numerous as they are compelling. Science targets range from exotic sources…

astro-ph.IM2015★ 164 cited

The low-frequency environment of the Murchison Widefield Array: radio-frequency interference analysis and mitigation

A. R. Offringa, R. B. Wayth, N. Hurley-Walker +62

The Murchison Widefield Array (MWA) is a new low-frequency interferometric radio telescope built in Western Australia at one of the locations of the future Square Kilometre Array (…

astro-ph.IM2014★ 937 cited

WSClean: an implementation of a fast, generic wide-field imager for radio astronomy

A. R. Offringa, B. McKinley, N. Hurley-Walker +50

Astronomical widefield imaging of interferometric radio data is computationally expensive, especially for the large data volumes created by modern non-coplanar many-element arrays.…