activity
19992021
most citedRevival of the magnetar PSR J1622-4950: observations with MeerKAT, Parkes, XMM-Newton, Swift, Chandra, and NuSTAR

161 citations · 539 across the 10 of their papers we have counts for

collaborators

10 papers

astro-ph.GA2021★ 130 cited

The MeerKAT Galaxy Cluster Legacy Survey I. Survey Overview and Highlights

K. Knowles, W. D. Cotton, L. Rudnick +148

MeerKAT's large number of antennas, spanning 8 km with a densely packed 1 km core, create a powerful instrument for wide-area surveys, with high sensitivity over a wide range of an…

astro-ph.GA2019★ 150 cited

Inflation of 430-parsec bipolar radio bubbles in the Galactic Centre by an energetic event

I. Heywood, F. Camilo, W. D. Cotton +96

The Galactic Centre contains a supermassive black hole with a mass of 4 million suns within an environment that differs markedly from that of the Galactic disk. While the black hol…

astro-ph.HE2018★ 161 cited

Revival of the magnetar PSR J1622-4950: observations with MeerKAT, Parkes, XMM-Newton, Swift, Chandra, and NuSTAR

F. Camilo, P. Scholz, M. Serylak +205

New radio (MeerKAT and Parkes) and X-ray (XMM-Newton, Swift, Chandra, and NuSTAR) observations of PSR J1622-4950 indicate that the magnetar, in a quiescent state since at least ear…

astro-ph.IM2016★ 37 cited

Engineering and Science Highlights of the KAT-7 Radio Telescope

A. R. Foley, T. Alberts, R P. Armstrong +100

The construction of the KAT-7 array in the Karoo region of the Northern Cape in South Africa was intended primarily as an engineering prototype for technologies and techniques appl…

astro-ph.HE2012★ 14 cited

PKS 2123-463: a confirmed gamma-ray blazar at high redshift

F. D'Ammando, A. Rau, P. Schady +11

The flat spectrum radio quasar (FSRQ) PKS 2123-463 was associated in the First Fermi-LAT source catalog with the gamma-ray source 1FGL J2126.1-4603, but when considering the full f…

astro-ph.SR2010★ 15 cited

Radio observations of candidate magnetic O stars

R. S. Schnerr, K. L. J. Rygl, A. J. van der Horst +5

Context: Some O stars are suspected to have to have (weak) magnetic fields because of the observed cyclical variability in their UV wind-lines. However, direct detections of these…