activity
20142023
most citedThe Rapid ASKAP Continuum Survey Paper II: First Stokes I Source Catalogue Data Release

189 citations · 1.8k across the 42 of their papers we have counts for

collaborators
Showing 2015Show all

6 papers · 1 filter

astro-ph.HE2015★ 7 cited

Orbital and superorbital variability of LS I +61 303 at low radio frequencies with GMRT and LOFAR

B. Marcote, M. Ribó, J. M. Paredes +23

LS I +61 303 is a gamma-ray binary that exhibits an outburst at GHz frequencies each orbital cycle of 26.5 d and a superorbital modulation with a period of 4.6…

astro-ph.HE2015★ 71 cited

LOFAR MSSS: Detection of a low-frequency radio transient in 400 hrs of monitoring of the North Celestial Pole

A. J. Stewart, R. P. Fender, J. W. Broderick +99

We present the results of a four-month campaign searching for low-frequency radio transients near the North Celestial Pole with the Low-Frequency Array (LOFAR), as part of the Mult…

astro-ph.HE2015★ 82 cited

Wide-Band, Low-Frequency Pulse Profiles of 100 Radio Pulsars with LOFAR

M. Pilia, J. W. T. Hessels, B. W. Stappers +84

LOFAR offers the unique capability of observing pulsars across the 10-240 MHz frequency range with a fractional bandwidth of roughly 50%. This spectral range is well-suited for stu…

astro-ph.IM2015★ 105 cited

The LOFAR Multifrequency Snapshot Sky Survey (MSSS) I. Survey description and first results

G. H. Heald, R. F. Pizzo, E. Orrú +147

We present the Multifrequency Snapshot Sky Survey (MSSS), the first northern-sky LOFAR imaging survey. In this introductory paper, we first describe in detail the motivation and de…

astro-ph.HE2015★ 13 cited

Transient Astrophysics with the Square Kilometre Array

Rob Fender, Adam Stewart, Jean-Pierre Macquart +5

This chapter provides an overview of the possibilities for transient and variable-source astrophysics with the Square Kilometre Array. While subsequent chapters focus on the astrop…

astro-ph.IM2015★ 2 cited

The LOFAR Transients Pipeline

John D. Swinbank, Tim D. Staley, Gijs J. Molenaar +23

Current and future astronomical survey facilities provide a remarkably rich opportunity for transient astronomy, combining unprecedented fields of view with high sensitivity and th…