activity
20052022
most citedLOFAR: The LOw-Frequency ARray

2.7k citations · 8.5k across the 97 of their papers we have counts for

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Showing 2014Show all

9 papers · 1 filter

astro-ph.IM2014★ 73 cited

Measuring a Cherenkov ring in the radio emission from air showers at 110-190 MHz with LOFAR

A. Nelles, P. Schellart, S. Buitink +66

Measuring radio emission from air showers offers a novel way to determine properties of the primary cosmic rays such as their mass and energy. Theory predicts that relativistic tim…

astro-ph.GA2014★ 26 cited

Discovery of Carbon Radio Recombination Lines in M82

Leah K. Morabito, J. B. R. Oonk, Francisco Salgado +30

Carbon radio recombination lines (RRLs) at low frequencies (<=500 MHz) trace the cold, diffuse phase of the interstellar medium, which is otherwise difficult to observe. We present…

physics.ins-det2014★ 62 cited

LORA: A scintillator array for LOFAR to measure extensive air showers

S. Thoudam, S. Buitink, A. Corstanje +11

The measurement of the radio emission from extensive air showers, induced by high-energy cosmic rays is one of the key science projects of the LOFAR radio telescope. The LOfar Radb…

astro-ph.IM2014★ 79 cited

Reconstruction of the energy and depth of maximum of cosmic-ray air-showers from LOPES radio measurements

W. D. Apel, J. C. Arteaga-Velazquez, L. Bähren +53

LOPES is a digital radio interferometer located at Karlsruhe Institute of Technology (KIT), Germany, which measures radio emission from extensive air showers at MHz frequencies in…

astro-ph.SR2014★ 78 cited

LOFAR tied-array imaging of Type III solar radio bursts

D. E. Morosan, P. T. Gallagher, P. Zucca +82

The Sun is an active source of radio emission which is often associated with energetic phenomena such as solar flares and coronal mass ejections (CMEs). At low radio frequencies (<…

astro-ph.GA2014★ 82 cited

Initial LOFAR observations of Epoch of Reionization windows: II. Diffuse polarized emission in the ELAIS-N1 field

V. Jelic, A. G. de Bruyn, M. Mevius +106

This study aims to characterise the polarized foreground emission in the ELAIS-N1 field and to address its possible implications for the extraction of the cosmological 21-cm signal…