activity
20072026
most citedLOFAR: The LOw-Frequency ARray

2.7k citations · 12.9k across the 158 of their papers we have counts for

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Showing 2021Show all

19 papers · 1 filter

astro-ph.GA2021★ 130 cited

The MeerKAT Galaxy Cluster Legacy Survey I. Survey Overview and Highlights

K. Knowles, W. D. Cotton, L. Rudnick +148

MeerKAT's large number of antennas, spanning 8 km with a densely packed 1 km core, create a powerful instrument for wide-area surveys, with high sensitivity over a wide range of an…

astro-ph.HE2021★ 54 cited

A snapshot of the oldest AGN feedback phases

M. Brienza, T. W. Shimwell, F. de Gasperin +19

Active Galactic Nuclei (AGN) inject large amounts of energy into their host galaxies and surrounding environment, shaping their properties and evolution. In particular, AGN jets in…

astro-ph.SR2021★ 90 cited

The population of M dwarfs observed at low radio frequencies

J. R. Callingham, H. K. Vedantham, T. W. Shimwell +12

Coherent low-frequency ( MHz) radio emission from stars encodes the conditions of the outer corona, mass-ejection events, and space weather. Previous low-frequency se…

astro-ph.GA2021★ 49 cited

The ultra-steep diffuse radio emission observed in the cool-core cluster RX J1720.1+2638 with LOFAR at 54 MHz

N. Biava, F. de Gasperin, A. Bonafede +17

Diffuse radio emission at the centre of galaxy clusters has been observed both in merging clusters on scales of Mpc, called giant radio haloes, and in relaxed systems with a cool-c…

astro-ph.GA2021

MIGHTEE: total intensity radio continuum imaging and the COSMOS / XMM-LSS Early Science fields

I. Heywood, M. J. Jarvis, C. L. Hale +23

MIGHTEE is a galaxy evolution survey using simultaneous radio continuum, spectro-polarimetry, and spectral line observations from the South African MeerKAT telescope. When complete…

astro-ph.GA2021★ 11 cited

The LOFAR LBA Sky Survey: Deep Fields I. The Boötes Field

W. L. Williams, F. de Gasperin, M. J. H. Hardcastle +9

We present the first sub-mJy ( mJy beam) survey to be completed below 100 MHz, which is over an order of magnitude deeper than previously achieved for widefield…