Abbott, B. and Abbott, R. and Adhikari, R. and Agresti, J. and Ajith, P. and Allen, B. and Allen, J. and Amin, R. and Anderson, S. B. and Anderson, W. G. and Araya, M. and Armandula, H. and Ashley, M. and Aulbert, C. and Babak, S. and Balasubramanian, R. and Ballmer, S. and Bantilan, H. and Barish, B. C. and Barker, C. and Barker, D. and Barton, M. A. and Bayer, K. and Belczynski, K. and Betzwieser, J. and Bhawal, B. and Bilenko, I. A. and Billingsley, G. and Black, E. and Blackburn, K. and Blackburn, L. and Bland, B. and Bogue, L. and Bork, R. and Bose, S. and Brady, P. R. and Braginsky, V. B. and Brau, J. E. and Brown, D. A. and Buonanno, A. and Busby, D. and Butler, W. E. and Cadonati, L. and Cagnoli, G. and Camp, J. B. and Cannizzo, J. and Cannon, K. and Cao, J. and Cardenas, L. and Carter, K. and Casey, M. M. and Charlton, P. and Chatterji, S. and Chen, Y. and Chin, D. and Christensen, N. and Cokelaer, T. and Colacino, C. N. and Coldwell, R. and Cook, D. and Corbitt, T. and Coyne, D. and Creighton, J. D. E. and Creighton, T. D. and Dalrymple, J. and D'Ambrosio, E. and Danzmann, K. and Davies, G. and DeBra, D. and Dergachev, V. and Desai, S. and DeSalvo, R. and Dhurandar, S. and Díaz, M. and Di Credico, A. and Drever, R. W. P. and Dupuis, R. J. and Ehrens, P. and Etzel, T. and Evans, M. and Evans, T. and Fairhurst, S. and Finn, L. S. and Franzen, K. Y. and Frey, R. E. and Fritschel, P. and Frolov, V. V. and Fyffe, M. and Ganezer, K. S. and Garofoli, J. and Gholami, I. and Giaime, J. A. and Goda, K. and Goggin, L. and González, G. and Gray, C. and Gretarsson, A. M. and Grimmett, D. and Grote, H. and Grunewald, S. and Guenther, M. and Gustafson, R. and Hamilton, W. O. and Hanna, C. and Hanson, J. and Hardham, C. and Harry, G. and Heefner, J. and Heng, I. S. and Hewitson, M. and Hindman, N. and Hoang, P. and Hough, J. and Hua, W. and Ito, M. and Itoh, Y. and Ivanov, A. and Johnson, B. and Johnson, W. W. and Jones, D. I. and Jones, G. and Jones, L. and Kalogera, V. and Katsavounidis, E. and Kawabe, K. and Kawamura, S. and Kells, W. and Khan, A. and Kim, C. and King, P. and Klimenko, S. and Koranda, S. and Kozak, D. and Krishnan, B. and Landry, M. and Lantz, B. and Lazzarini, A. and Lei, M. and Leonor, I. and Libbrecht, K. and Lindquist, P. and Liu, S. and Lormand, M. and Lubinski, M. and Lück, H. and Luna, M. and Machenschalk, B. and MacInnis, M. and Mageswaran, M. and Mailand, K. and Malec, M. and Mandic, V. and Márka, S. and Maros, E. and Mason, K. and Matone, L. and Mavalvala, N. and McCarthy, R. and McClelland, D. E. and McHugh, M. and McNabb, J. W. C. and Melissinos, A. and Mendell, G. and Mercer, R. A. and Meshkov, S. and Messaritaki, E. and Messenger, C. and Mikhailov, E. and Mitra, S. and Mitrofanov, V. P. and Mitselmakher, G. and Mittleman, R. and Miyakawa, O. and Mohanty, S. and Moreno, G. and Mossavi, K. and Mueller, G. and Mukherjee, S. and Myers, E. and Myers, J. and Nash, T. and Nocera, F. and Noel, J. S. and O'Reilly, B. and O'Shaughnessy, R. and Ottaway, D. J. and Overmier, H. and Owen, B. J. and Pan, Y. and Papa, M. A. and Parameshwaraiah, V. and Parameswariah, C. and Pedraza, M. and Penn, S. and Pitkin, M. and Prix, R. and Quetschke, V. and Raab, F. and Radkins, H. and Rahkola, R. and Rakhmanov, M. and Rawlins, K. and Ray-Majumder, S. and Re, V. and Regimbau, T. and Reitze, D. H. and Riesen, R. and Riles, K. and Rivera, B. and Robertson, D. I. and Robertson, N. A. and Robinson, C. and Roddy, S. and Rodriguez, A. and Rollins, J. and Romano, J. D. and Romie, J. and Rowan, S. and Rüdiger, A. and Ruet, L. and Russell, P. and Ryan, K. and Sandberg, V. and Sanders, G. H. and Sannibale, V. and Sarin, P. and Sathyaprakash, B. S. and Saulson, P. R. and Savage, R. and Sazonov, A. and Schilling, R. and Schofield, R. and Schutz, B. F. and Schwinberg, P. and Scott, S. M. and Seader, S. E. and Searle, A. C. and Sears, B. and Sellers, D. and Sengupta, A. S. and Shawhan, P. and Shoemaker, D. H. and Sibley, A. and Siemens, X. and Sigg, D. and Sintes, A. M. and Smith, J. and Smith, M. R. and Spjeld, O. and Strain, K. A. and Strom, D. M. and Stuver, A. and Summerscales, T. and Sung, M. and Sutton, P. J. and Tanner, D. B. and Tarallo, M. and Taylor, R. and Thorne, K. A. and Thorne, K. S. and Tokmakov, K. V. and Torres, C. and Torrie, C. and Traylor, G. and Tyler, W. and Ugolini, D. and Ungarelli, C. and Vallisneri, M. and van Putten, M. and Vass, S. and Vecchio, A. and Veitch, J. and Vorvick, C. and Vyachanin, S. P. and Wallace, L. and Ward, H. and Ward, R. and Watts, K. and Webber, D. and Weiland, U. and Weinstein, A. and Weiss, R. and Wen, S. and Wette, K. and Whelan, J. T. and Whitcomb, S. E. and Whiting, B. F. and Wiley, S. and Wilkinson, C. and Willems, P. A. and Willke, B. and Wilson, A. and Winkler, W. and Wise, S. and Wiseman, A. G. and Woan, G. and Woods, D. and Wooley, R. and Worden, J. and Yakushin, I. and Yamamoto, H. and Yoshida, S. and Zanolin, M. and Zhang, L. and Zotov, N. and Zucker, M. 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:ABBcqg06
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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 Institute of Physics and IOP Publishing Limited. Received 14 October 2005, in final form 29 November 2005. Published 22 March 2006. Print publication: Issue 8 (21 April 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:||ROTATIONAL CORE COLLAPSE; PERFORMANCE|
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|Usage Policy:||No commercial reproduction, distribution, display or performance rights in this work are provided.|
|Deposited By:||Tony Diaz|
|Deposited On:||15 Jan 2009 00:24|
|Last Modified:||20 Mar 2013 18:09|
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