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|a Wipf, Christopher C.
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|a Massachusetts Institute of Technology. Department of Physics
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|a MIT Kavli Institute for Astrophysics and Space Research
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|a Mavalvala, Nergis
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|a Zucker, Michael E.
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|a Wipf, Christopher C.
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|a Weiss, Rainer
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|a Waldman, Samuel J.
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|a Stein, Leo Chaim
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|a Stein, Andrew J.
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|a Smith, Nicolas de Mateo
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|a Shoemaker, David H.
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|a Shapiro, B.
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|a Sarin, P.
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|a Mittleman, Richard K.
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|a Mason, Kenneth R.
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|a Markowitz, Jared John
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|a MacInnis, Myron E.
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|a Katsavounidis, Erotokritos
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|a Hughey, Brennan J.
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|a Harry, Gregory
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|a Grimaldi, F.
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|a Goda, K.
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|a Fritschel, Peter K.
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|a Foley, Stephany
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|a Evans, Matthew J.
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|a Duke, I.
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|a Donovan, Frederick J.
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|a Corbitt, Thomas R.
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|a Cao, Junwei
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|a Brunet, G.
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|a Bodiya, Timothy Paul
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|a Blackburn, Lindy L.
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|a Barsotti, Lisa
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|a Mavalvala, Nergis
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|a Weiss, Rainer
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|a Waldman, Samuel J.
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|a Stein, Leo Chaim
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|a Stein, Andrew J.
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|a Smith, Nicolas de Mateo
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|a Shapiro, B.
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|a Sarin, P.
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|a Markowitz, Jared John
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|a Katsavounidis, Erotokritos
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|a Hughey, Brennan J.
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|a Harry, Gregory
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|a Grimaldi, F.
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|a Goda, K.
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|a Foley, Stephany
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|a Duke, I.
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|a Cao, Junwei
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|a Brunet, G.
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|a Blackburn, Lindy L.
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|a Barsotti, Lisa
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|a Mavalvala, Nergis
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|a Zucker, Michael E
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|a Mittleman, Richard K
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|a Corbitt, Thomas R
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|a Shoemaker, David H
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|a Mason, Kenneth R
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|a MacInnis, Myron E
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|a Fritschel, Peter K
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|a Evans, Matthew J
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|a Donovan, Frederick J
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|a Bodiya, Timothy P.
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|a Search for gravitational waves from low mass compact binary coalescence in 186 days of LIGO's fifth science run
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|b American Physical Society,
|c 2010-03-01T15:30:30Z.
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|z Get fulltext
|u http://hdl.handle.net/1721.1/51842
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|a We report on a search for gravitational waves from coalescing compact binaries, of total mass between 2 and 35M[subscript ⊙], 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[superscript -2], 7.3×10[superscript -4] and 3.6×10[superscript -3] yr[superscript -1] L[subscript 10][superscript -1], respectively, where L[subscript 10] is 10[superscript 10] times the blue solar luminosity.
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|a Alfred P. Sloan Foundation
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|a Research Corporation
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|a David and Lucile Packard Foundation
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|a Leverhulme Trust
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|a Carnegie Trust
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|a National Aeronautics and Space Administration
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|a Scottish Universities Physics Alliance
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|a Scottish Funding Council
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|a Royal Society, United Kingdom
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|a Conselleria d'Economia, Hisenda i Innovació of the Govern de les Illes Balears
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|a Ministerio de Ciencia e Innovación, Spain
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|a Istituto Nazionale di Fisica Nucleare of Italy
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|a Council of Scientific and Industrial Research of India
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|a Australian Research Council
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|a State of Niedersachsen/Germany
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|a Max Planck Society for the Advancement of Science
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|a Science and Technology Facilities Council, United Kingdom
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|a National Science Foundation
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|a en_US
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|a Article
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|t Physical Review D
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