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Published April 21, 2006 | Published
Journal Article Open

Search for gravitational-wave bursts in LIGO's third science run

Abbott, B.
Abbott, R.
Adhikari, Rana X.
Agresti, J.
Ajith, P.
Allen, B.
Allen, J.
Amin, R.
Anderson, S. B.
Anderson, W. G.
Araya, M.
Armandula, H.
Ashley, M.
Aulbert, C.
Babak, S.
Balasubramanian, R.
Ballmer, S.
Bantilan, H.
Barish, B. C.
Barker, C.
Barker, D.
Barton, M. A.
Bayer, K.
Belczynski, K.
Betzwieser, J.
Bhawal, B.
Bilenko, I. A.
Billingsley, G.
Black, E.
Blackburn, K.
Blackburn, L.
Bland, B.
Bogue, L.
Bork, R.
Bose, S.
Brady, P. R.
Braginsky, V. B.
Brau, J. E.
Brown, D. A.
Buonanno, A.
Busby, D.
Butler, W. E.
Cadonati, L.
Cagnoli, G.
Camp, J. B.
Cannizzo, J.
Cannon, K.
Cao, J.
Cardenas, L.
Carter, K.
Casey, M. M.
Charlton, P.
Chatterji, S.
Chen, Y.
Chin, D.
Christensen, N.
Cokelaer, T.
Colacino, C. N.
Coldwell, R.
Cook, D.
Corbitt, T.
Coyne, D.
Creighton, J. D. E.
Creighton, T. D.
Dalrymple, J.
D'Ambrosio, E.
Danzmann, K.
Davies, G.
DeBra, D.
Dergachev, V.
Desai, S.
DeSalvo, R.
Dhurandar, S.
Díaz, M.
Di Credico, A.
Drever, R. W. P.
Dupuis, R. J.
Ehrens, P.
Etzel, T.
Evans, M.
Evans, T.
Fairhurst, S.
Finn, L. S.
Franzen, K. Y.
Frey, R. E.
Fritschel, P.
Frolov, V. V.
Fyffe, M.
Ganezer, K. S.
Garofoli, J.
Gholami, I.
Giaime, J. A.
Goda, K.
Goggin, L.
González, G.
Gray, C.
Gretarsson, A. M.
Grimmett, D.
Grote, H.
Grunewald, S.
Guenther, M.
Gustafson, R.
Hamilton, W. O.
Hanna, C.
Hanson, J.
Hardham, C.
Harry, G.
Heefner, J.
Heng, I. S.
Hewitson, M.
Hindman, N.
Hoang, P.
Hough, J.
Hua, W.
Ito, M.
Itoh, Y.
Ivanov, A.
Johnson, B.
Johnson, W. W.
Jones, D. I.
Jones, G.
Jones, L.
Kalogera, V.
Katsavounidis, E.
Kawabe, K.
Kawamura, S.
Kells, W.
Khan, A.
Kim, C.
King, P.
Klimenko, S.
Koranda, S.
Kozak, D.
Krishnan, B.
Landry, M.
Lantz, B.
Lazzarini, A.
Lei, M.
Leonor, I.
Libbrecht, K.
Lindquist, P.
Liu, S.
Lormand, M.
Lubinski, M.
Lück, H.
Luna, M.
Machenschalk, B.
MacInnis, M.
Mageswaran, M.
Mailand, K.
Malec, M.
Mandic, V.
Márka, S.
Maros, E.
Mason, K.
Matone, L.
Mavalvala, N.
McCarthy, R.
McClelland, D. E.
McHugh, M.
McNabb, J. W. C.
Melissinos, A.
Mendell, G.
Mercer, R. A.
Meshkov, S.
Messaritaki, E.
Messenger, C.
Mikhailov, E.
Mitra, S.
Mitrofanov, V. P.
Mitselmakher, G.
Mittleman, R.
Miyakawa, O.
Mohanty, S.
Moreno, G.
Mossavi, K.
Mueller, G.
Mukherjee, S.
Myers, E.
Myers, J.
Nash, T.
Nocera, F.
Noel, J. S.
O'Reilly, B.
O'Shaughnessy, R.
Ottaway, D. J.
Overmier, H.
Owen, B. J.
Pan, Y.
Papa, M. A.
Parameshwaraiah, V.
Parameswariah, C.
Pedraza, M.
Penn, S.
Pitkin, M.
Prix, R.
Quetschke, V.
Raab, F.
Radkins, H.
Rahkola, R.
Rakhmanov, M.
Rawlins, K.
Ray-Majumder, S.
Re, V.
Regimbau, T.
Reitze, D. H.
Riesen, R.
Riles, K.
Rivera, B.
Robertson, D. I.
Robertson, N. A.
Robinson, C.
Roddy, S.
Rodriguez, A.
Rollins, J.
Romano, J. D.
Romie, J. H.
Rowan, S.
Rüdiger, A.
Ruet, L.
Russell, P.
Ryan, K.
Sandberg, V.
Sanders, G. H.
Sannibale, V.
Sarin, P.
Sathyaprakash, B. S.
Saulson, P. R.
Savage, R.
Sazonov, A.
Schilling, R.
Schofield, R.
Schutz, B. F.
Schwinberg, P.
Scott, S. M.
Seader, S. E.
Searle, A. C.
Sears, B.
Sellers, D.
Sengupta, A. S.
Shawhan, P.
Shoemaker, D. H.
Sibley, A.
Siemens, X.
Sigg, D.
Sintes, A. M.
Smith, J.
Smith, M. R.
Spjeld, O.
Strain, K. A.
Strom, D. M.
Stuver, A.
Summerscales, T.
Sung, M.
Sutton, P. J.
Tanner, D. B.
Tarallo, M.
Taylor, R.
Thorne, K. A.
Thorne, K. S.
Tokmakov, K. V.
Torres, C.
Torrie, C.
Traylor, G.
Tyler, W.
Ugolini, D.
Ungarelli, C.
Vallisneri, M.
van Putten, M.
Vass, S.
Vecchio, A.
Veitch, J.
Vorvick, C.
Vyachanin, S. P.
Wallace, L.
Ward, H.
Ward, R.
Watts, K.
Webber, D.
Weiland, U.
Weiss, R.
Wen, S.
Wette, K.
Whelan, J. T.
Whitcomb, S. E.
Whiting, B. F.
Wiley, S.
Wilkinson, C.
Willems, P. A.
Willke, B.
Wilson, A.
Winkler, W.
Wise, S.
Wiseman, A. G.
Woan, G.
Woods, D.
Wooley, R.
Worden, J.
Yakushin, I.
Yamamoto, H.
Yoshida, S.
Zanolin, M.
Zhang, L.
Zotov, N.
Zucker, M.
Zweizig, J.
Weinstein, Alan J.
LIGO Scientific Collaboration

Abstract

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.

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