activity
20062026
most citedSearch for an isotropic gravitational-wave background with the Parkes Pulsar Timing Array

1.2k citations · 13.1k across the 120 of their papers we have counts for

collaborators
Showing 2017 · astro-ph.HEShow all

6 papers · 2 filters

astro-ph.HE2017★ 1 cited

X-rays from the mode-switching PSR B0943+10

S. Mereghetti, L. Kuiper, A. Tiengo +15

New simultaneous X-ray and radio observations of the archetypal mode-switching pulsar PSR B0943+10 have been carried out with XMM-Newton and the LOFAR, LWA and Arecibo radio telesc…

astro-ph.HE2017★ 75 cited

Inferring the population properties of binary neutron stars with gravitational-wave measurements of spin

Xing-Jiang Zhu, Eric Thrane, Stefan Osłowski +2

The recent LIGO-Virgo detection of gravitational waves from a binary neutron star inspiral event GW170817 and the discovery of its accompanying electromagnetic signals mark a new e…

astro-ph.HE2017★ 212 cited

Follow up of GW170817 and its electromagnetic counterpart by Australian-led observing programs

I. Andreoni, K. Ackley, J. Cooke +122

The discovery of the first electromagnetic counterpart to a gravitational wave signal has generated follow-up observations by over 50 facilities world-wide, ushering in the new era…

astro-ph.HE2017★ 8 cited

Limits on the Mass, Velocity and Orbit of PSR J19336211

E. Graikou, J. P. W. Verbiest, S. Oslowski +4

We present a high-precision timing analysis of PSR J19336211, a millisecond pulsar (MSP) with a 3.5-ms spin period and a white dwarf (WD) companion, using data from the Parkes r…

astro-ph.HE2017★ 165 cited

The detection of an extremely bright fast radio burst in a phased array feed survey

Keith Bannister, Ryan Shannon, Jean-Pierre Macquart +53

We report the detection of an ultra-bright fast radio burst (FRB) from a modest, 3.4-day pilot survey with the Australian Square Kilometre Array Pathfinder. The survey was conducte…

astro-ph.HE2017★ 29 cited

Comparison of Pulsar Positions from Timing and Very Long Baseline Astrometry

J. B. Wang, W. A. Coles, G. Hobbs +22

Pulsar positions can be measured with high precision using both pulsar timing methods and very-long-baseline interferometry (VLBI). Pulsar timing positions are referenced to a sola…