activity
20062015
most citedThe Murchison Widefield Array: the Square Kilometre Array Precursor at low radio frequencies

1.3k citations · 2.9k across the 21 of their papers we have counts for

collaborators

22 papers

astro-ph.IM2015★ 28 cited

A Digital-Receiver for the Murchison Widefield Array

Thiagaraj Prabu, K. S. Srivani, D. Anish Roshi +55

An FPGA-based digital-receiver has been developed for a low-frequency imaging radio interferometer, the Murchison Widefield Array (MWA). The MWA, located at the Murchison Radio-ast…

astro-ph.IM2015★ 42 cited

The Murchison Widefield Array Correlator

S. M. Ord, B. Crosse, D. Emrich +64

The Murchison Widefield Array (MWA) is a Square Kilometre Array (SKA) Precursor. The telescope is located at the Murchison Radio--astronomy Observatory (MRO) in Western Australia (…

astro-ph.IM2014★ 2 cited

Observing the Sun with the Murchison Widefield Array

D. Oberoi, R. Sharma, S. Bhatnagar +42

The Sun has remained a difficult source to image for radio telescopes, especially at the low radio frequencies. Its morphologically complex emission features span a large range of…

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…