activity
19972019
most citedThe Murchison Widefield Array: the Square Kilometre Array Precursor at low radio frequencies

1.3k citations · 7.6k across the 51 of their papers we have counts for

collaborators

52 papers

astro-ph.IM2019★ 1.1k cited

First M87 Event Horizon Telescope Results. II. Array and Instrumentation

The Event Horizon Telescope Collaboration

The Event Horizon Telescope (EHT) is a very long baseline interferometry (VLBI) array that comprises millimeter- and submillimeter-wavelength telescopes separated by distances comp…

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…

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.IM2016★ 72 cited

The Murchison Widefield Array 21 cm Power Spectrum Analysis Methodology

Daniel C. Jacobs, B. J. Hazelton, C. M. Trott +61

We present the 21 cm power spectrum analysis approach of the Murchison Widefield Array Epoch of Reionization project. In this paper, we compare the outputs of multiple pipelines fo…

astro-ph.CO2016★ 110 cited

First Limits on the 21 cm Power Spectrum during the Epoch of X-ray heating

A. Ewall-Wice, Joshua S. Dillon, J. N. Hewitt +62

We present first results from radio observations with the Murchison Widefield Array seeking to constrain the power spectrum of 21 cm brightness temperature fluctuations between the…