activity
20062023
most citedLOFAR: The LOw-Frequency ARray

2.7k citations · 5.6k across the 42 of their papers we have counts for

collaborators

44 papers

astro-ph.IM2023★ 6 cited

Apertif 1.4 GHz continuum observations of the Boötes field and their combined view with LOFAR

A. M. Kutkin, T. A. Oosterloo, R. Morganti +17

We present a new image of a 26.5 square degree region in the Boötes constellation obtained at 1.4 GHz using the Aperture Tile in Focus (Apertif) system on the Westerbork Synthesis…

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.GA2021★ 35 cited

Sub-arcsecond imaging with the International LOFAR Telescope: II. Completion of the LOFAR Long-Baseline Calibrator Survey

Neal Jackson, Shruti Badole, John Morgan +69

The Low-Frequency Array (LOFAR) Long-Baseline Calibrator Survey (LBCS) was conducted between 2014 and 2019 in order to obtain a set of suitable calibrators for the LOFAR array. In…

astro-ph.IM2021★ 88 cited

Sub-arcsecond imaging with the International LOFAR Telescope I. Foundational calibration strategy and pipeline

L. K. Morabito, N. J. Jackson, S. Mooney +71

[abridged] The International LOFAR Telescope is an interferometer with stations spread across Europe. With baselines of up to ~2,000 km, LOFAR has the unique capability of achievin…

astro-ph.IM2020

Mid Frequency Aperture Array Architectural Design Document

A. W. Gunst, A. J. Faulkner, S. Wijnholds +3

The Square Kilometre Array (SKA) is the next generation radio telescope. Aperture Arrays (AA) are considered for SKA-2 for frequencies up to 1.4 GHz (SKA-1 uses AAs up to 350 MHz).…

astro-ph.HE2020★ 11 cited

LOFAR 144-MHz follow-up observations of GW170817

J. W. Broderick, T. W. Shimwell, K. Gourdji +66

We present low-radio-frequency follow-up observations of AT 2017gfo, the electromagnetic counterpart of GW170817, which was the first binary neutron star merger to be detected by A…