activity
20132025
most citedProbing Atmospheric Electric Fields in Thunderstorms through Radio Emission from Cosmic-Ray-Induced Air Showers

55 citations · 272 across the 12 of their papers we have counts for

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6 papers · 1 filter

astro-ph.IM2025

Real-time station monitor and stationtest pipelines for LOFAR 2.0

Jun Wang, M. J. Norden, P. Donker

LOFAR is a low-frequency array distributed across several European countries. Each LOFAR station contains thousands of antennas and associated electronics, making monitoring and th…

astro-ph.IM2022★ 14 cited

Continuum source catalog for the first APERTIF data release

A. M. Kutkin, T. A. Oosterloo, R. Morganti +25

The first data release of Apertif survey contains 3074 radio continuum images covering a thousand square degrees of the sky. The observations were performed during August 2019 to J…

astro-ph.IM2022★ 42 cited

First release of Apertif imaging survey data

Elizabeth A. K. Adams, B. Adebahr, W. J. G. de Blok +56

(Abridged) Apertif is a phased-array feed system for WSRT, providing forty instantaneous beams over 300 MHz of bandwidth. A dedicated survey program started on 1 July 2019, with th…

astro-ph.IM2022★ 6 cited

Characterising the Apertif primary beam response

H. Dénes, K. M. Hess, E. A. K. Adams +27

Context. Phased Array Feeds (PAFs) are multi element receivers in the focal plane of a telescope that make it possible to form simultaneously multiple beams on the sky by combining…

astro-ph.IM2021

Apertif, Phased Array Feeds for the Westerbork Synthesis Radio Telescope

W. A. van Cappellen, T. A. Oosterloo, M. A. W. Verheijen +87

We describe the APERture Tile In Focus (Apertif) system, a phased array feed (PAF) upgrade of the Westerbork Synthesis Radio Telescope which has transformed this telescope into a h…

astro-ph.IM2021

The LOFAR LBA Sky Survey I. survey description and preliminary data release

F. de Gasperin, W. L. Williams, P. Best +38

LOFAR is the only radio telescope that is presently capable of high-sensitivity, high-resolution (<1 mJy/b and <15") observations at ultra-low frequencies (<100 MHz). To utilise th…