activity
20042020
most citedObserving pulsars and fast transients with LOFAR

218 citations · 1.7k across the 21 of their papers we have counts for

collaborators
Showing 2014Show all

6 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.IM2014★ 38 cited

The LOFAR long baseline snapshot calibrator survey

J. Moldón, A. T. Deller, O. Wucknitz +82

Aims. An efficient means of locating calibrator sources for International LOFAR is developed and used to determine the average density of usable calibrator sources on the sky for s…

astro-ph.GA2014★ 30 cited

LOFAR observations of PSR B0943+10: profile evolution and discovery of a systematically changing profile delay in Bright mode

A. Bilous, J. Hessels, V. Kondratiev +10

We present broadband, low-frequency (25-80 MHz and 110-190 MHz) LOFAR observations of PSR B0943+10, with the goal of better illuminating the nature of its enigmatic mode-switching…

astro-ph.SR2014★ 104 cited

The LOFAR Pilot Surveys for Pulsars and Fast Radio Transients

Thijs Coenen, Joeri van Leeuwen, Jason W. T. Hessels +87

We have conducted two pilot surveys for radio pulsars and fast transients with the Low-Frequency Array (LOFAR) around 140 MHz and here report on the first low-frequency fast-radio…

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.HE2014★ 39 cited

On the Apparent Nulls and Extreme Variability of PSR J1107-5907

N. J. Young, P. Weltevrede, B. W. Stappers +2

We present an analysis of the emission behaviour of PSR J1107-5907, a source known to exhibit separate modes of emission, using observations obtained over approximately 10 yr. We f…