activity
20122019
most citedFirst M87 Event Horizon Telescope Results. II. Array and Instrumentation

1.1k citations · 1.2k across the 7 of their papers we have counts for

collaborators

13 papers

astro-ph.IM20191.1k 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.GA201618 cited

A Large Scale, Low Frequency Murchison Widefield Array Survey of Galactic HII regions between 260< l <\340

L. Hindson, M. Johnston-Hollitt, N. Hurley-Walker +40

We have compiled a catalogue of HII regions detected with the Murchison Widefield Array (MWA) between 72 and 231MHz. The multiple frequency bands provided by the MWA allow us ident…

astro-ph.HE2016

Time-domain and spectral properties of pulsars at 154 MHz

M. E. Bell, Tara Murphy, S. Johnston +35

We present 154 MHz Murchison Widefield Array imaging observations and variability information for a sample of pulsars. Over the declination range we…

astro-ph.CO2016

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…

astro-ph.IM2016

The 154 MHz radio sky observed by the Murchison Widefield Array: noise, confusion and first source count analyses

T. M. O. Franzen, C. A. Jackson, A. R. Offringa +30

We analyse a 154 MHz image made from a 12 h observation with the Murchison Widefield Array (MWA) to determine the noise contribution and behaviour of the source counts down to 30 m…

astro-ph.HE2016

High-energy sources at low radio frequency: the Murchison Widefield Array view of Fermi blazars

M. Giroletti, F. Massaro, R. D'Abrusco +54

Low-frequency radio arrays are opening a new window for the study of the sky, both to study new phenomena and to better characterize known source classes. Being flat-spectrum sourc…