activity
20102016
most citedLOFAR: The LOw-Frequency ARray

2.7k citations · 3.7k across the 18 of their papers we have counts for

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Showing 2013Show all

7 papers · 1 filter

astro-ph.CO2013★ 3 cited

Probing the accelerating Universe with radio weak lensing in the JVLA Sky Survey

M. L. Brown, F. B. Abdalla, A. Amara +48

We outline the prospects for performing pioneering radio weak gravitational lensing analyses using observations from a potential forthcoming JVLA Sky Survey program. A large-scale…

astro-ph.IM2013★ 63 cited

RESOLVE: A new algorithm for aperture synthesis imaging of extended emission in radio astronomy

H. Junklewitz, M. R. Bell, M. Selig +1

We present RESOLVE, a new algorithm for radio aperture synthesis imaging of extended and diffuse emission in total intensity. The algorithm is derived using Bayesian statistical in…

astro-ph.CO2013★ 17 cited

The brightness and spatial distributions of terrestrial radio sources

A. R. Offringa, A. G. de Bruyn, S. Zaroubi +75

Faint undetected sources of radio-frequency interference (RFI) might become visible in long radio observations when they are consistently present over time. Thereby, they might obs…

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…