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

1.3k citations · 9.9k across the 132 of their papers we have counts for

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Showing astro-ph.GAShow all

14 papers · 1 filter

astro-ph.GA2019★ 5 cited

Astro2020 Science White Paper: Synergies Between Galaxy Surveys and Reionization Measurements

Steven Furlanetto, Adam Beardsley, Chris L. Carilli +47

The early phases of galaxy formation constitute one of the most exciting frontiers in astrophysics. It is during this era that the first luminous sources reionize the intergalactic…

astro-ph.GA2019★ 6 cited

Cosmic Dawn and Reionization: Astrophysics in the Final Frontier

Asantha Cooray, James Aguirre, Yacine Ali-Haimoud +71

The cosmic dawn and epoch of reionization mark the time period in the universe when stars, galaxies, and blackhole seeds first formed and the intergalactic medium changed from neut…

astro-ph.GA2017★ 35 cited

Spectral energy distribution and radio halo of NGC 253 at low radio frequencies

A. D. Kapinska, L. Staveley-Smith, R. Crocker +67

We present new radio continuum observations of NGC253 from the Murchison Widefield Array at frequencies between 76 and 227 MHz. We model the broadband radio spectral energy distrib…

astro-ph.GA2016★ 557 cited

GaLactic and Extragalactic All-sky Murchison Widefield Array (GLEAM) survey I: A low-frequency extragalactic catalogue

Natasha Hurley-Walker, Joseph R. Callingham, Paul J. Hancock +40

Using the Murchison Widefield Array (MWA), the low-frequency Square Kilometre Array (SKA1 LOW) precursor located in Western Australia, we have completed the GaLactic and Extragalac…

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.GA2016★ 11 cited

The radio spectral energy distribution of infrared-faint radio sources

A. Herzog, R. P. Norris, E. Middelberg +57

Infrared-faint radio sources (IFRS) are a class of radio-loud (RL) active galactic nuclei (AGN) at high redshifts (z > 1.7) that are characterised by their relative infrared faintn…