Document Type

Article

Publication Date

2009

Abstract

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 L−110, respectively, where L10 is 1010 times the blue solar luminosity.

Comments

©2009 American Physical Society. Original published version available at https://doi.org/10.1103/PhysRevD.80.047101

Publication Title

Physical Review D

DOI

10.1103/PhysRevD.80.047101

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