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most citedParameter estimation for compact binary coalescence signals with the first generation gravitational-wave detector network

160 citations · 1.2k across the 19 of their papers we have counts for

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gr-qc2015★ 25 cited

Parameter choices and ranges for continuous gravitational wave searches for steadily spinning neutron stars

D. I. Jones

We consider the issue of selecting parameters and their associated ranges for carrying out searches for continuous gravitational waves from steadily rotating neutron stars. We cons…

gr-qc2013★ 160 cited

Parameter estimation for compact binary coalescence signals with the first generation gravitational-wave detector network

the LIGO Scientific Collaboration, the Virgo Collaboration, J. Aasi +801

Compact binary systems with neutron stars or black holes are one of the most promising sources for ground-based gravitational wave detectors. Gravitational radiation encodes rich i…

gr-qc2007★ 73 cited

Are neutron stars with crystalline colour superconducting cores interesting for the LIGO experiment?

B. Haskell, N. Andersson, D. I. Jones +1

We estimate the maximal deformation that can be sustained by a rotating neutron star with a crystalline colour superconducting quark core. Our results suggest that current gravitat…

gr-qc2004★ 17 cited

Bounding the mass of the graviton using eccentric binaries

D I Jones

We describe a method by which gravitational wave observations of eccentric binary systems could be used to test General Relativity's prediction that gravitational waves are dispers…

gr-qc2001★ 132 cited

Gravitational waves from freely precessing neutron stars

D. I. Jones, N. Andersson

In this paper we model the gravitational wave emission of a freely precessing neutron star. The aim is to estimate likely source strengths, as a guide for gravitational wave astron…