activity
20112021
most citedLOFAR: The LOw-Frequency ARray

2.7k citations · 5k across the 30 of their papers we have counts for

collaborators

31 papers

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.SR2018★ 85 cited

Shock location and CME 3D reconstruction of a solar type II radio burst with LOFAR

P. Zucca, D. E. Morosan, A. P. Rouillard +62

Type II radio bursts are evidence of shocks in the solar atmosphere and inner heliosphere that emit radio waves ranging from sub-meter to kilometer lengths. These shocks may be ass…

astro-ph.IM2016★ 74 cited

LBCS: the LOFAR Long-Baseline Calibrator Survey

N. Jackson, A. Tagore, A. Deller +76

(abridged). We outline LBCS (the LOFAR Long-Baseline Calibrator Survey), whose aim is to identify sources suitable for calibrating the highest-resolution observations made with the…

astro-ph.HE2016★ 156 cited

A large light-mass component of cosmic rays at 10^{17} - 10^{17.5} eV from radio observations

S. Buitink, A. Corstanje, H. Falcke +101

Cosmic rays are the highest energy particles found in nature. Measurements of the mass composition of cosmic rays between 10^{17} eV and 10^{18} eV are essential to understand whet…

astro-ph.HE2015★ 71 cited

LOFAR MSSS: Detection of a low-frequency radio transient in 400 hrs of monitoring of the North Celestial Pole

A. J. Stewart, R. P. Fender, J. W. Broderick +99

We present the results of a four-month campaign searching for low-frequency radio transients near the North Celestial Pole with the Low-Frequency Array (LOFAR), as part of the Mult…

astro-ph.EP2015★ 53 cited

Imaging Jupiter's radiation belts down to 127 MHz with LOFAR

J. N. Girard, P. Zarka, C. Tasse +71

Context. Observing Jupiter's synchrotron emission from the Earth remains today the sole method to scrutinize the distribution and dynamical behavior of the ultra energetic electron…