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|a Zucker, Michael E.
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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 Mavalvala, Nergis
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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 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 Mavalvala, Nergis
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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 Search for gravitational-wave bursts in the first year of the fifth LIGO science run
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|b American Physical Society,
|c 2010-03-18T18:19:28Z.
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|z Get fulltext
|u http://hdl.handle.net/1721.1/52714
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|a We present the results obtained from an all-sky search for gravitational-wave (GW) bursts in the 64-2000 Hz frequency range in data collected by the LIGO detectors during the first year (November 2005-November 2006) of their fifth science run. The total analyzed live time was 268.6 days. Multiple hierarchical data analysis methods were invoked in this search. The overall sensitivity expressed in terms of the root-sum-square (rss) strain amplitude h[subscript rss] for gravitational-wave bursts with various morphologies was in the range of 6×10[superscript -22] Hz[superscript -1/2] to a few×10-[superscript 21] Hz[superscript -1/2]. No GW signals were observed and a frequentist upper limit of 3.75 events per year on the rate of strong GW bursts was placed at the 90% confidence level. As in our previous searches, we also combined this rate limit with the detection efficiency for selected waveform morphologies to obtain event rate versus strength exclusion curves. In sensitivity, these exclusion curves are the most stringent to date.
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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 Spanish Ministerio de Educación y Ciencia
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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 in Germany
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|a Max-Planck-Society
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|a Science and Technology Facilities Council of the 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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