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20092026
most citedLOFAR: The LOw-Frequency ARray

2.7k citations · 8.3k across the 74 of their papers we have counts for

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22 papers · 1 filter

astro-ph.GA2023

Radio multifrequency observations of Abell~781 with the WSRT

B. V. Hugo, G. Bernardi, O. M. Smirnov +4

The `Main' galaxy cluster in the Abell 781 system is undergoing a significant merger and accretion process with peripheral emission to the north and southeastern flanks of the merg…

astro-ph.GA2021★ 35 cited

Sub-arcsecond imaging with the International LOFAR Telescope: II. Completion of the LOFAR Long-Baseline Calibrator Survey

Neal Jackson, Shruti Badole, John Morgan +69

The Low-Frequency Array (LOFAR) Long-Baseline Calibrator Survey (LBCS) was conducted between 2014 and 2019 in order to obtain a set of suitable calibrators for the LOFAR array. In…

astro-ph.GA2021★ 69 cited

LOFAR imaging of Cygnus A -- Direct detection of a turnover in the hotspot radio spectra

J. P. McKean, L. E. H. Godfrey, S. Vegetti +75

The low-frequency radio spectra of the hotspots within powerful radio galaxies can provide valuable information about the physical processes operating at the site of the jet termin…

astro-ph.GA2020★ 86 cited

The beautiful mess in Abell 2255

A. Botteon, G. Brunetti, R. J. van Weeren +18

We present LOFAR observations of one of the most spectacular objects in the radio sky: Abell 2255. This is a nearby () merging galaxy cluster hosting one of the first r…

astro-ph.GA2019★ 163 cited

A radio ridge connecting two galaxy clusters in a filament of the cosmic web

F. Govoni, E. Orrù, A. Bonafede +26

Galaxy clusters are the most massive gravitationally bound structures in the Universe. They grow by accreting smaller structures in a merging process that produces shocks and turbu…

astro-ph.GA2018★ 586 cited

The LOFAR Two-metre Sky Survey - II. First data release

T. W. Shimwell, C. Tasse, M. J. Hardcastle +104

The LOFAR Two-metre Sky Survey (LoTSS) is an ongoing sensitive, high-resolution 120-168MHz survey of the entire northern sky for which observations are now 20% complete. We present…