Abbott, B. and Abbott, R. and Adhikari, R. and Agresti, J. and Anderson, S. B. and Araya, M. and Armandula, H. and Barish, B. C. and Barton, M. A. and Bhawal, B. and Billingsley, G. and Black, E. and Blackburn, K. and Bork, R. and Brown, D. A. and Busby, D. and Cardenas, L. and Charlton, P. and Chatterji, S. and Coyne, D. and Creighton, T. D. and D'Ambrosio, E. and DeSalvo, R. and Drever, R. W. P. and Dupuis, R. J. and Ehrens, P. and Etzel, T. and Evans, M. and Goggin, L. and Grimmett, D. and Heefner, J. and Ivanov, A. and Jones, L. and Kells, W. and King, P. and Kozak, D. and Lazzarini, A. and Lei, M. and Libbrecht, K. and Lindquist, P. and Liu, S. and Mageswaran, M. and Mailand, K. and Mandic, V. and Maros, E. and Meshkov, S. and Miyakawa, O. and Nash, T. and Nocera, F. and Pedraza, M. and Romie, J. and Russell, P. and Sanders, G. H. and Sannibale, V. and Sears, B. and Shawhan, P. and Sutton, P. J. and Smith, M. R. and Tarallo, M. and Taylor, R. and Torrie, C. and Thorne, K. S. and Tyler, W. and Vallisneri, M. and Vass, S. and Wallace, L. and Ward, R. and Webber, D. and Weinstein, A. and Whitcomb, S. E. and Willems, P. A. and Wilson, A. and Yamamoto, H. and Zhang, L. and Zweizig, J. (2006) Search for gravitational-wave bursts in LIGO’s third science run. Classical and Quantum Gravity, 23 (8). S29-S39. ISSN 0264-9381 http://resolver.caltech.edu/CaltechAUTHORS:20100512-142729349
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We report on a search for gravitational-wave bursts in data from the three LIGO interferometric detectors during their third science run. The search targets subsecond bursts in the frequency range 100–1100 Hz for which no waveform model is assumed and has a sensitivity in terms of the root-sum-square (rss) strain amplitude of h_(rss) ∼ 10^(−20) Hz^(−1/2). No gravitational-wave signals were detected in the eight days of analysed data.
|Additional Information:||© 2006 IOP Publishing Ltd. Received 14 October 2005, in final form 29 November 2005. Published 22 March 2006. The authors gratefully acknowledge the support of the United States National Science Foundation for the construction and operation of the LIGO Laboratory, and the Particle Physics and Astronomy Research Council of the United Kingdom, the Max-Planck-Society and the State of Niedersachsen/Germany for support of the construction and operation of the GEO600 detector. The authors also gratefully acknowledge the support of the research by these agencies and by the Australian Research Council, the Natural Sciences and Engineering Research Council of Canada, the Council of Scientific and Industrial Research of India, the Department of Science and Technology of India, the Spanish Ministerio de Educacion y Ciencia, the John Simon Guggenheim Foundation, the Leverhulme Trust, the David and Lucile Packard Foundation, the Research Corporation and the Alfred P Sloan Foundation. This paper has been assigned LIGO Laboratory document number P050043-A-R.|
|Subject Keywords:||Instrumentation and measurement; Gravitation and cosmology; Astrophysics and astroparticles|
|Other Numbering System:|
|Classification Code:||PACS: 04.80.Nn, 07.05.Kf, 95.30.Sf, 95.85.Sz. MSC: 83C35.|
|Official Citation:||B Abbott et al 2006 Class. Quantum Grav. 23 S29 doi: 10.1088/0264-9381/23/8/S05|
|Usage Policy:||No commercial reproduction, distribution, display or performance rights in this work are provided.|
|Deposited By:||Ruth Sustaita|
|Deposited On:||21 May 2010 15:36|
|Last Modified:||26 Dec 2012 12:02|
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