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

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Showing astro-ph.GAShow all

9 papers · 1 filter

astro-ph.GA2019★ 49 cited

First detection of frequency-dependent, time-variable dispersion measures

J. Y. Donner, J. P. W. Verbiest, C. Tiburzi +11

Context. High-precision pulsar-timing experiments are affected by temporal variations of the Dispersion Measure (DM), which are related to spatial variations in the interstellar el…

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…

astro-ph.GA2014★ 108 cited

Searching for gravitational wave memory bursts with the Parkes Pulsar Timing Array

J. B. Wang, G. Hobbs, W. Coles +17

Anisotropic bursts of gravitational radiation produced by events such as super-massive black hole mergers leave permanent imprints on space. Such gravitational wave "memory" (GWM)…

astro-ph.GA2014★ 138 cited

An all-sky search for continuous gravitational waves in the Parkes Pulsar Timing Array data set

X. -J. Zhu, G. Hobbs, L. Wen +16

We present results of an all-sky search in the Parkes Pulsar Timing Array (PPTA) Data Release 1 data set for continuous gravitational waves (GWs) in the frequency range from $5\tim…

astro-ph.GA2012★ 224 cited

Measurement and correction of variations in interstellar dispersion in high-precision pulsar timing

M. J. Keith, W. Coles, R. M. Shannon +16

Signals from radio pulsars show a wavelength-dependent delay due to dispersion in the interstellar plasma. At a typical observing wavelength, this delay can vary by tens of microse…

astro-ph.GA2011★ 84 cited

High signal-to-noise ratio observations and the ultimate limits of precision pulsar timing

Stefan Oslowski, Willem van Straten, George Hobbs +2

We demonstrate that the sensitivity of high-precision pulsar timing experiments will be ultimately limited by the broadband intensity modulation that is intrinsic to the pulsar's s…