activity
20102026
most citedThe Murchison Widefield Array: the Square Kilometre Array Precursor at low radio frequencies

1.3k citations · 6k across the 65 of their papers we have counts for

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Showing 2013Show all

7 papers · 1 filter

astro-ph.GA2013★ 67 cited

A survey for transients and variables with the Murchison Widefield Array 32-tile prototype at 154 MHz

M. E. Bell, T. Murphy, D. L. Kaplan +55

We present a search for transient and variable radio sources at 154 MHz with the Murchison Widefield Array 32-tile prototype. Fifty-one images were obtained that cover a field of v…

astro-ph.CO2013★ 165 cited

A study of fundamental limitations to statistical detection of redshifted HI from the epoch of reionization

Nithyanandan Thyagarajan, N. Udaya Shankar, Ravi Subrahmanyan +46

In this paper we explore for the first time the relative magnitudes of three fundamental sources of uncertainty, namely, foreground contamination, thermal noise and sample variance…

astro-ph.CO2013★ 27 cited

The giant lobes of Centaurus A observed at 118 MHz with the Murchison Widefield Array

B. McKinley, F. Briggs, B. M. Gaensler +50

We present new wide-field observations of Centaurus A (Cen A) and the surrounding region at 118 MHz with the Murchison Widefield Array (MWA) 32-tile prototype, with which we invest…

astro-ph.IM2013★ 52 cited

On the detection and tracking of space debris using the Murchison Widefield Array. I. Simulations and test observations demonstrate feasibility

S. J. Tingay, D. L. Kaplan, B. McKinley +60

The Murchison Widefield Array (MWA) is a new low frequency interferomeric radio telescope. The MWA is the low frequency precursor to the Square Kilometre Array (SKA) and is the fir…

astro-ph.CO2013★ 102 cited

A 189 MHz, 2400 square degree polarization survey with the Murchison Widefield Array 32-element prototype

G. Bernardi, L. J. Greenhill, D. A. Mitchell +50

We present a Stokes I, Q and U survey at 189 MHz with the Murchison Widefield Array 32-element prototype covering 2400 square degrees. The survey has a 15.6 arcmin angular resoluti…

astro-ph.CO2013★ 191 cited

Overcoming real-world obstacles in 21 cm power spectrum estimation: A method demonstration and results from early Murchison Widefield Array data

Joshua S. Dillon, Adrian Liu, Christopher L. Williams +16

We present techniques for bridging the gap between idealized inverse covariance weighted quadratic estimation of 21 cm power spectra and the real-world challenges presented univers…