activity
20092026
most citedThe Murchison Widefield Array: the Square Kilometre Array Precursor at low radio frequencies

1.3k citations · 6.6k across the 70 of their papers we have counts for

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Showing astro-ph.COShow all

10 papers · 1 filter

astro-ph.CO2023★ 111 cited

The second data release from the European Pulsar Timing Array: IV. Implications for massive black holes, dark matter and the early Universe

J. Antoniadis, P. Arumugam, S. Arumugam +111

The European Pulsar Timing Array (EPTA) and Indian Pulsar Timing Array (InPTA) collaborations have measured a low-frequency common signal in the combination of their second and fir…

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.CO2015★ 53 cited

A search for Fast Radio Bursts at low frequencies with Murchison Widefield Array high time resolution imaging

S. J. Tingay, C. M. Trott, R. B. Wayth +26

We present the results of a pilot study search for Fast Radio Bursts (FRBs) using the Murchison Widefield Array (MWA) at low frequencies (139 - 170 MHz). We utilised MWA data obtai…

astro-ph.CO2015★ 95 cited

Confirmation of Wide-Field Signatures in Redshifted 21 cm Power Spectra

Nithyanandan Thyagarajan, Daniel C. Jacobs, Judd D. Bowman +52

We confirm our recent prediction of the "pitchfork" foreground signature in power spectra of high-redshift 21 cm measurements where the interferometer is sensitive to large-scale s…

astro-ph.CO2015★ 122 cited

Empirical Covariance Modeling for 21 cm Power Spectrum Estimation: A Method Demonstration and New Limits from Early Murchison Widefield Array 128-Tile Data

Joshua S. Dillon, Abraham R. Neben, Jacqueline N. Hewitt +52

The separation of the faint cosmological background signal from bright astrophysical foregrounds remains one of the most daunting challenges of mapping the high-redshift intergalac…

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…