activity
20122018
most citedRevival of the magnetar PSR J1622-4950: observations with MeerKAT, Parkes, XMM-Newton, Swift, Chandra, and NuSTAR

161 citations · 328 across the 6 of their papers we have counts for

collaborators

7 papers

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.SR2015

LOFAR discovery of a quiet emission mode in PSR B0823+26

C. Sobey, N. J. Young, J. W. T. Hessels +91

PSR B0823+26, a 0.53-s radio pulsar, displays a host of emission phenomena over timescales of seconds to (at least) hours, including nulling, subpulse drifting, and mode-changing.…

astro-ph.HE2015★ 32 cited

Long-term Observations of Three Nulling Pulsars

N. J. Young, P. Weltevrede, B. W. Stappers +2

We present an analysis of approximately 200 hours of observations of the pulsars J16345107, J17174054 and J18530505, taken over the course of 14.7 yr. We show that all of…

astro-ph.HE2014★ 39 cited

On the Apparent Nulls and Extreme Variability of PSR J1107-5907

N. J. Young, P. Weltevrede, B. W. Stappers +2

We present an analysis of the emission behaviour of PSR J1107-5907, a source known to exhibit separate modes of emission, using observations obtained over approximately 10 yr. We f…

astro-ph.HE2012★ 30 cited

Long-term Radio Observations of the Intermittent Pulsar B1931+24

N. J. Young, B. W. Stappers, A. G. Lyne +3

We present an analysis of approximately 13-yr of observations of the intermittent pulsar B1931+24 to further elucidate its behaviour. We find that while the source exhibits a wide…