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

354 citations · 1k across the 8 of their papers we have counts for

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astro-ph200837 cited

PSR J1856+0245: Arecibo Discovery of a Young, Energetic Pulsar Coincident with the TeV Gamma-ray Source HESS J1857+026

J. W. T. Hessels, D. J. Nice, B. M. Gaensler +21

We present the discovery of the Vela-like radio pulsar J1856+0245 in the Arecibo PALFA survey. PSR J1856+0245 has a spin period of 81ms, a characteristic age of 21kyr, and a spin-d…

astro-ph2008193 cited

An Eccentric Binary Millisecond Pulsar in the Galactic Plane

D. J. Champion, S. M. Ransom, P. Lazarus +28

Binary pulsar systems are superb probes of stellar and binary evolution and the physics of extreme environments. In a survey with the Arecibo telescope, we have found PSR J1903+032…

astro-ph2007152 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-ph2006354 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…

astro-ph2006170 cited

Measurement of Orbital Decay in the Double Neutron Star Binary PSR B2127+11C

B. A. Jacoby, P. B. Cameron, F. A. Jenet +3

We report the direct measurement of orbital period decay in the double neutron star pulsar system PSR B2127+11C in the globular cluster M15 at the rate of $(-3.95 \pm 0.13) \times…

astro-ph2005

Pulsar timing and the detection of black hole binary systems in globular clusters

Fredrick A. Jenet, Teviet Creighton, Andrea Lommen

The possible existence of intermediate mass binary black holes (IMBBHs) in globular clusters (GCs) offers a unique geometry in which to detect space-time oscillations. For certain…