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19992015
most citedTEMPO2, a new pulsar timing package. I: Overview

1.2k citations · 4.1k across the 26 of their papers we have counts for

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astro-ph2008★ 3 cited

The Subpulse Modulation Properties of Pulsars and its Frequency Dependence

Patrick Weltevrede, Ben Stappers, R. T. Edwards

A large sample of about two hundred pulsars have been observed to study their subpulse modulation at an observing wavelength of (when achievable) both 21 and 92 cm using the Wester…

astro-ph2008★ 292 cited

Precision timing of PSR J0437-4715: an accurate pulsar distance, a high pulsar mass and a limit on the variation of Newton's gravitational constant

J. P. W. Verbiest, M. Bailes, W. van Straten +7

Analysis of ten years of high-precision timing data on the millisecond pulsar PSR J0437-4715 has resulted in a model-independent kinematic distance based on an apparent orbital per…

astro-ph2007★ 134 cited

The subpulse modulation properties of pulsars at 92 cm and the frequency dependence of subpulse modulation

P. Weltevrede, B. W. Stappers, R. T. Edwards

A large sample of pulsars has been observed to study their subpulse modulation at an observing wavelength (when achievable) of both 21 and 92 cm using the Westerbork Synthesis Radi…

astro-ph2007★ 152 cited

Dispersion Measure Variations and their Effect on Precision Pulsar Timing

X. P. You, G. Hobbs, W. A. Coles +11

We present an analysis of the variations seen in the dispersion measures (DMs) of 20 millisecond pulsars observed as part of the Parkes Pulsar Timing Array project. We carry out a…

astro-ph2007

Drifting subpulse survey at 21 cm

P. Weltevrede, R. T. Edwards, B. W. Stappers

We present the statistical results of a systematic, unbiased search for subpulse modulation of 187 pulsars performed with the Westerbork Synthesis Radio Telescope (WSRT) in the Net…

astro-ph2006★ 354 cited

Upper bounds on the low-frequency stochastic gravitational wave background from pulsar timing observations: current limits and future prospects

F. A. Jenet, G. B. Hobbs, W. van Straten +7

Using a statistically rigorous analysis method, we place limits on the existence of an isotropic stochastic gravitational wave background using pulsar timing observations. We consi…