activity
20042021
most citedLOFAR: The LOw-Frequency ARray

2.7k citations · 9.1k across the 107 of their papers we have counts for

collaborators

108 papers

astro-ph.GA2021★ 33 cited

CHANG-ES XXIII: Influence of a galactic wind in NGC 5775

G. H. Heald, V. Heesen, S. S. Sridhar +22

We present new radio continuum images of the edge-on starburst galaxy NGC 5775, from LOFAR (140 MHz) and the Karl G. Jansky Very Large Array CHANG-ES survey (1500 MHz). We trace th…

astro-ph.GA2021★ 189 cited

The Rapid ASKAP Continuum Survey Paper II: First Stokes I Source Catalogue Data Release

C. L. Hale, D. McConnell, A. J. M. Thomson +10

The Rapid ASKAP Continuum Survey (RACS) is the first large sky survey using the Australian Square Kilometre Array Pathfinder (ASKAP), covering the sky south of +41 declinat…

astro-ph.HE2021★ 28 cited

Discovery of ASKAP J173608.2-321635 as a Highly-Polarized Transient Point Source with the Australian SKA Pathfinder

Ziteng Wang, David L. Kaplan, Tara Murphy +18

We report the discovery of a highly-polarized, highly-variable, steep-spectrum radio source, ASKAP J173608.2-321635, located 4\,deg from the Galactic center in the Galactic p…

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.HE2021★ 4 cited

The ASKAP Variables and Slow Transients (VAST) Pilot Survey

Tara Murphy, David L. Kaplan, Adam J. Stewart +52

The Variables and Slow Transients Survey (VAST) on the Australian Square Kilometre Array Pathfinder (ASKAP) is designed to detect highly variable and transient radio sources on tim…

astro-ph.IM2021★ 100 cited

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…