activity
20132018
most citedCalibrating High-Precision Faraday Rotation Measurements for LOFAR and the Next Generation of Low-Frequency Radio Telescopes

161 citations · 409 across the 7 of their papers we have counts for

collaborators

9 papers

astro-ph.GA201878 cited

Radio haloes in nearby galaxies modelled with 1D cosmic-ray transport using SPINNAKER

V. Heesen, M. Krause, R. Beck +10

We present radio continuum maps of 12 nearby (), edge-on (), late-type spiral galaxies mostly at and 5 GHz, observed with the Australia Te…

astro-ph.IM201714 cited

Source Finding in Linear Polarization for LOFAR, and SKA Predecessor Surveys, using Faraday Moments

J. S. Farnes, G. Heald, H. Junklewitz +10

The optimal source-finding strategy for linear polarization data is an unsolved problem, with many inhibitive factors imposed by the technically-challenging nature of polarization…

astro-ph.GA201782 cited

Deep LOFAR observations of the merging galaxy cluster CIZA J2242.8+5301

D. N. Hoang, T. W. Shimwell, A. Stroe +20

Previous studies have shown that CIZA J2242.8+5301 (the 'Sausage' cluster, ) is a massive merging galaxy cluster that hosts a radio halo and multiple relics. In this paper…

astro-ph.GA201719 cited

LOFAR MSSS: The Scaling Relation between AGN Cavity Power and Radio Luminosity at Low Radio Frequencies

G. Kokotanekov, M. Wise, G. H. Heald +35

We present a new analysis of the widely used relation between cavity power and radio luminosity in clusters of galaxies with evidence for strong AGN feedback. We study the correlat…

astro-ph.HE2016

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.SR2015

LOFAR discovery of a quiet emission mode in PSR B0823+26

C. Sobey, N. J. Young, J. W. T. Hessels +91

PSR B0823+26, a 0.53-s radio pulsar, displays a host of emission phenomena over timescales of seconds to (at least) hours, including nulling, subpulse drifting, and mode-changing.…