activity
20102017
most citedLOFAR: The LOw-Frequency ARray

2.7k citations · 3.4k across the 13 of their papers we have counts for

collaborators

14 papers

astro-ph.GA2017★ 43 cited

The population of SNe/SNRs in the starburst galaxy Arp 220. A self-consistent analysis of 20 years of VLBI monitoring

E. Varenius, J. E. Conway, F. Batejat +6

The nearby ultra-luminous infrared galaxy (ULIRG) Arp 220 is an excellent laboratory for studies of extreme astrophysical environments. For 20 years, Very Long Baseline Interferome…

astro-ph.GA2014★ 20 cited

Discovery of Carbon Radio Recombination Lines in absorption towards Cygnus~A

J. B. R. Oonk, R. J. van Weeren, F. Salgado +100

We present the first detection of carbon radio recombination line absorption along the line of sight to Cygnus A. The observations were carried out with the LOw Frequency ARray in…

astro-ph.IM2013★ 2.7k cited

LOFAR: The LOw-Frequency ARray

M. P. van Haarlem, M. W. Wise, A. W. Gunst +197

LOFAR, the LOw-Frequency ARray, is a new-generation radio interferometer constructed in the north of the Netherlands and across europe. Utilizing a novel phased-array design, LOFAR…

astro-ph.GA2013★ 20 cited

LOFAR detections of low-frequency radio recombination lines towards Cassiopeia A

Ashish Asgekar, J. B. R. Oonk, S. Yatawatta +89

Cassiopeia A was observed using the Low-Band Antennas of the LOw Frequency ARray (LOFAR) with high spectral resolution. This allowed a search for radio recombination lines (RRLs) a…

astro-ph.SR2013★ 32 cited

Differential Frequency-dependent Delay from the Pulsar Magnetosphere

T. E. Hassall, B. W. Stappers, P. Weltevrede +60

Some radio pulsars show clear drifting subpulses, in which subpulses are seen to drift in pulse longitude in a systematic pattern. Here we examine how the drifting subpulses of PSR…

astro-ph.HE2013★ 134 cited

Synchronous X-ray and Radio Mode Switches: a Rapid Global Transformation of the Pulsar Magnetosphere

W. Hermsen, J. W. T. Hessels, L. Kuiper +8

Pulsars emit low-frequency radio waves through to high-energy gamma-rays that are generated anywhere from the surface out to the edges of the magnetosphere. Detecting correlated mo…

astro-ph.IM2013★ 159 cited

Initial deep LOFAR observations of Epoch of Reionization windows: I. The North Celestial Pole

S. Yatawatta, A. G. de Bruyn, M. A. Brentjens +86

The aim of the LOFAR Epoch of Reionization (EoR) project is to detect the spectral fluctuations of the redshifted HI 21cm signal. This signal is weaker by several orders of magnitu…

astro-ph.CO2012★ 10 cited

Rapid variability of the compact radio sources in Arp220. Evidence for a population of microblazars?

F. Batejat, J. E. Conway, A. Rushton +3

Context. The two nuclei of the starburst galaxy Arp220 contain multiple compact radio sources previously identified as radio supernovae or supernova remnants. Aims. In order to sea…

astro-ph.CO2012★ 18 cited

e-MERLIN and VLBI observations of the luminous infrared galaxy IC883: a nuclear starburst and an AGN candidate revealed

C. Romero-Canizales, M. A. Perez-Torres, A. Alberdi +11

The high star formation rates of luminous infrared galaxies (LIRGs) make them ideal places for core-collapse supernova (CCSN) searches. At radio frequencies, free from dust extinct…

astro-ph.CO2011★ 47 cited

Resolution of the Compact Radio Continuum Sources in Arp220

Fabien Batejat, John E. Conway, Rossa Hurley +4

We present 2 cm and 3.6 cm wavelength very long baseline interferometry images of the compact radio continuum sources in the nearby ultra-luminous infrared galaxy Arp220. Based on…

astro-ph.CO2011★ 59 cited

LOFAR and APERTIF surveys of the radio sky: probing shocks and magnetic fields in galaxy clusters

Huub Rottgering, Jose Afonso, Peter Barthel +32

At very low frequencies, the new pan-European radio telescope LOFAR is opening the last unexplored window of the electromagnetic spectrum for astrophysical studies. The revolutiona…

astro-ph.CO2011★ 6 cited

LOFAR: Early imaging results from commissioning for Cygnus A

John McKean, Louise Ker, Reinout J. van Weeren +19

The Low Frequency Array (LOFAR) will operate between 10 and 250 MHz, and will observe the low frequency Universe to an unprecedented sensitivity and angular resolution. The constru…

astro-ph.CO2011★ 138 cited

Molecules as tracers of galaxy evolution: an EMIR survey. I. Presentation of the data and first results

F. Costagliola, S. Aalto, M. I. Rodriguez +10

We investigate the molecular gas properties of a sample of 23 galaxies in order to find and test chemical signatures of galaxy evolution and to compare them to IR evolutionary trac…

astro-ph.CO2010

Compact source resolution and rapid variability in Arp220

Fabien Batejat, John E. Conway, Philip J. Diamond +3

We present multi-epoch global VLBI observations at 2 cm, 3.6 cm and 6 cm of the compact radio sources in Arp220. We resolve many sources and estimate sizes, expansion velocities an…