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Phys. Rev. D 80, 047101 (2009) [8 pages]

Search for gravitational waves from low mass compact binary coalescence in 186 days of LIGO’s fifth science run

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B. P. Abbott et al. LIGO Scientific Collaboration
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Received 18 June 2009; published 25 August 2009

We report on a search for gravitational waves from coalescing compact binaries, of total mass between 2 and 35M, using LIGO observations between November 14, 2006 and May 18, 2007. No gravitational-wave signals were detected. We report upper limits on the rate of compact binary coalescence as a function of total mass. The LIGO cumulative 90%-confidence rate upper limits of the binary coalescence of neutron stars, black holes and black hole-neutron star systems are 1.4×10-2, 7.3×10-4 and 3.6×10-3  yr-1 L10-1, respectively, where L10 is 1010 times the blue solar luminosity.

© 2009 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevD.80.047101
DOI:
10.1103/PhysRevD.80.047101
PACS:
95.85.Sz, 04.80.Nn, 07.05.Kf, 97.60.Jd