activity
20092025
most citedThe LOFAR Two-metre Sky Survey -- V. Second data release

489 citations · 2k across the 48 of their papers we have counts for

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7 papers · 1 filter

astro-ph.HE2020

Reaching thermal noise at ultra-low radio frequencies: the Toothbrush radio relic downstream of the shock front

F. de Gasperin, G. Brunetti, M. Bruggen +14

Ultra-low frequency observations (<100 MHz) are particularly challenging because they are usually performed in a low signal-to-noise ratio regime due to the high sky temperature an…

astro-ph.HE2020

Cassiopeia A, Cygnus A, Taurus A, and Virgo A at ultra-low radio frequencies

F. de Gasperin, J. Vink, J. P. McKean +49

The four persistent radio sources in the northern sky with the highest flux density at metre wavelengths are Cassiopeia A, Cygnus A, Taurus A, and Virgo A; collectively they are ca…

astro-ph.HE201927 cited

New candidate radio supernova remnants detected in the GLEAM survey over ,

Natasha Hurley-Walker, Miroslav D. Filipovic, Bryan M. Gaensler +18

We have detected 27 new supernova remnants (SNRs) using a new data release of the GLEAM survey from the Murchison Widefield Array (MWA) telescope, including the lowest surface-brig…

astro-ph.HE201935 cited

Candidate radio supernova remnants observed by the GLEAM survey over and

Natasha Hurley-Walker, Bryan M. Gaensler, Denis A. Leahy +18

We examined the latest data release from the GaLactic and Extragalactic All-sky Murchison Widefield Array (GLEAM) survey covering , $180^\circ < l < 240^\…

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.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…