activity
20152026
most citedSearch for an isotropic gravitational-wave background with the Parkes Pulsar Timing Array

1.2k citations · 7.4k across the 82 of their papers we have counts for

collaborators
Showing 2015Show all

6 papers · 1 filter

astro-ph.CO2015★ 195 cited

Gravitational-wave cosmology across 29 decades in frequency

Paul D. Lasky, Chiara M. F. Mingarelli, Tristan L. Smith +24

Quantum fluctuations of the gravitational field in the early Universe, amplified by inflation, produce a primordial gravitational-wave background across a broad frequency band. We…

astro-ph.IM2015★ 40 cited

Versatile Directional Searches for Gravitational Waves with Pulsar Timing Arrays

D. R. Madison, X. -J. Zhu, G. Hobbs +23

By regularly monitoring the most stable millisecond pulsars over many years, pulsar timing arrays (PTAs) are positioned to detect and study correlations in the timing behaviour of…

astro-ph.HE2015★ 4 cited

Timing analysis for 20 millisecond pulsars in the Parkes Pulsar Timing Array

D. J. Reardon, G. Hobbs, W. Coles +18

We present timing models for 20 millisecond pulsars in the Parkes Pulsar Timing Array. The precision of the parameter measurements in these models has been improved over earlier re…

astro-ph.CO2015★ 494 cited

Gravitational waves from binary supermassive black holes missing in pulsar observations

R. M. Shannon, V. Ravi, L. T. Lentati +19

Gravitational waves are expected to be radiated by supermassive black hole binaries formed during galaxy mergers. A stochastic superposition of gravitational waves from all such bi…

astro-ph.SR2015★ 101 cited

Pulsar Observations of Extreme Scattering Events

W. A. Coles, M. Kerr, R. M. Shannon +17

Extreme scattering events (ESEs) in the interstellar medium (ISM) were first observed in regular flux measurements of compact extragalactic sources. They are characterized by a flu…

astro-ph.GA2015★ 157 cited

A Study of Multi-frequency Polarization Pulse Profiles of Millisecond Pulsars

S. Dai, G. Hobbs, R. N. Manchester +23

We present high signal-to-noise ratio, multi-frequency polarization pulse profiles for 24 millisecond pulsars that are being observed as part of the Parkes Pulsar Timing Array (PPT…