activity
20102016
most citedLOFAR: The LOw-Frequency ARray

2.7k citations · 3.3k across the 10 of their papers we have counts for

collaborators

11 papers

astro-ph.IM2016★ 1 cited

Operations in the era of large distributed telescopes

Yan Guillaume Grange, Kevin Vinsen, Juan Carlos Guzman +4

The previous generation of astronomical instruments tended to consist of single receivers in the focal point of one or more physical reflectors. Because of this, most astronomical…

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★ 125 cited

Detecting cosmic rays with the LOFAR radio telescope

P. Schellart, A. Nelles, S. Buitink +102

The low frequency array (LOFAR), is the first radio telescope designed with the capability to measure radio emission from cosmic-ray induced air showers in parallel with interferom…

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.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…