Journal
PHYSICAL REVIEW D
Volume 80, Issue 4, Pages -Publisher
AMER PHYSICAL SOC
DOI: 10.1103/PhysRevD.80.047101
Keywords
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Funding
- United States National Science Foundation
- LIGO Laboratory
- Science and Technology Facilities Council of the United Kingdom
- Max-Planck-Society
- State of Niedersachsen/Germany
- Division Of Physics
- Direct For Mathematical & Physical Scien [0905184, 0757058] Funding Source: National Science Foundation
- Division Of Physics
- Direct For Mathematical & Physical Scien [855313, 0855679] Funding Source: National Science Foundation
- Science and Technology Facilities Council [ST/F01032X/1, PP/F001096/1, PP/F00110X/1, PP/F001118/1, ST/G504284/1, PP/E001203/1] Funding Source: researchfish
- STFC [PP/F001118/1, ST/G504284/1, PP/F00110X/1, ST/F01032X/1, PP/E001203/1, PP/F001096/1] Funding Source: UKRI
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We report on a search for gravitational waves from coalescing compact binaries, of total mass between 2 and 35M(circle dot), 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 1.4x10(-2), 7.3x10(-4) and 3.6x10(-3) yr(-1) L-10(-1), respectively, where L-10 is 10(10) times the blue solar luminosity.
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