Please use this identifier to cite or link to this item: http://hdl.handle.net/2440/48824
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Type: Journal article
Title: Analysis of LIGO data for gravitational waves from binary neutron stars
Author: Abbott, B.
Abbott, R.
Adhikari, R.
Allen, B.
Amin, R.
Anderson, S.
Anderson, W.
Araya, M.
Armandula, H.
Asiri, F.
Aufmuth, P.
Aulbert, C.
Babak, S.
Balasubramanian, R.
Ballmer, S.
Barish, B.
Barker, D.
Barker, C.
Barnes, M.
Barr, B.
et al.
Citation: Physical Review. D. Particles, Fields, Gravitation and Cosmology, 2004; 69(12):122001-1-122001-16
Publisher: American Physical Soc
Issue Date: 2004
ISSN: 1550-7998
2470-0029
Statement of
Responsibility: 
B. Abbott...D. Ottaway...C. Killow...et al., LIGO Scientific Collaboration
Abstract: We report on a search for gravitational waves from coalescing compact binary systems in the Milky Way and the Magellanic Clouds. The analysis uses data taken by two of the three LIGO interferometers during the first LIGO science run and illustrates a method of setting upper limits on inspiral event rates using interferometer data. The analysis pipeline is described with particular attention to data selection and coincidence between the two interferometers. We establish an observational upper limit of R<1.7×102 per year per Milky Way Equivalent Galaxy (MWEG), with 90% confidence, on the coalescence rate of binary systems in which each component has a mass in the range 1–3M⊙.
Keywords: General Relativity and Quantum Cosmology (gr-qc)
Rights: ©2004 American Physical Society.
RMID: 0020083087
DOI: 10.1103/PhysRevD.69.122001
Appears in Collections:Physics publications

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