B Abbott et al 2006 Class. Quantum Grav. 23 S29 doi:10.1088/0264-9381/23/8/S05
B Abbott1, R Abbott1, R Adhikari1, J Agresti1, P Ajith2, B Allen3, J Allen4, R Amin5, S B Anderson1, W G Anderson3, M Araya1, H Armandula1, M Ashley6, C Aulbert7, S Babak7, R Balasubramanian8, S Ballmer4, H Bantilan9, B C Barish1, C Barker10, D Barker10, M A Barton1, K Bayer4, K Belczynski11,42, J Betzwieser4, B Bhawal1, I A Bilenko12, G Billingsley1, E Black1, K Blackburn1, L Blackburn4, B Bland10, L Bogue13, R Bork1, S Bose14, P R Brady3, V B Braginsky12, J E Brau15, D A Brown1, A Buonanno16, D Busby1, W E Butler17, L Cadonati4, G Cagnoli18, J B Camp19, J Cannizzo19, K Cannon3, J Cao4, L Cardenas1, K Carter13, M M Casey18, P Charlton1,43, S Chatterji1, Y Chen7, D Chin20, N Christensen9, T Cokelaer8, C N Colacino21, R Coldwell22, D Cook10, T Corbitt4, D Coyne1, J D E Creighton3, T D Creighton1, J Dalrymple23, E D'Ambrosio1, K Danzmann2,24, G Davies8, D DeBra25, V Dergachev20, S Desai6, R DeSalvo1, S Dhurandar35, M Díaz26, A Di Credico23, R W P Drever27, R J Dupuis1, P Ehrens1, T Etzel1, M Evans1, T Evans13, S Fairhurst3, L S Finn6, K Y Franzen22, R E Frey15, P Fritschel4, V V Frolov13, M Fyffe13, K S Ganezer28, J Garofoli10, I Gholami7, J A Giaime5, K Goda4, L Goggin1, G González5, C Gray10, A M Gretarsson29, D Grimmett1, H Grote2, S Grunewald7, M Guenther10, R Gustafson20, W O Hamilton5, C Hanna5, J Hanson13, C Hardham25, G Harry4, J Heefner1, I S Heng18, M Hewitson2, N Hindman10, P Hoang1, J Hough18, W Hua25, M Ito15, Y Itoh3, A Ivanov1, B Johnson10, W W Johnson5, D I Jones6,44, G Jones8, L Jones1, V Kalogera11, E Katsavounidis4, K Kawabe10, S Kawamura30, W Kells1, A Khan13, C Kim11, P King1, S Klimenko22, S Koranda3, D Kozak1, B Krishnan7, M Landry10, B Lantz25, A Lazzarini1, M Lei1, I Leonor15, K Libbrecht1, P Lindquist1, S Liu1, M Lormand13, M Lubinski10, H Lück2, M Luna31, B Machenschalk7, M MacInnis4, M Mageswaran1, K Mailand1, M Malec24, V Mandic1, S Márka32, E Maros1, K Mason4, L Matone32, N Mavalvala4, R McCarthy10, D E McClelland33, M McHugh34, J W C McNabb6, A Melissinos17, G Mendell10, R A Mercer21, S Meshkov1, E Messaritaki3, C Messenger21, E Mikhailov4, S Mitra35, V P Mitrofanov12, G Mitselmakher22, R Mittleman4, O Miyakawa1, S Mohanty26, G Moreno10, K Mossavi2, G Mueller22, S Mukherjee26, E Myers36, J Myers10, T Nash1, F Nocera1, J S Noel14, B O'Reilly13, R O'Shaughnessy11, D J Ottaway4, H Overmier13, B J Owen6, Y Pan37, M A Papa7, V Parameshwaraiah10, C Parameswariah13,45, M Pedraza1, S Penn38, M Pitkin18, R Prix7, V Quetschke22, F Raab10, H Radkins10, R Rahkola15, M Rakhmanov22, K Rawlins4,46, S Ray-Majumder3, V Re21, T Regimbau8,47, D H Reitze22, R Riesen13, K Riles20, B Rivera10, D I Robertson18, N A Robertson18,25, C Robinson8, S Roddy13, A Rodriguez5, J Rollins32, J D Romano8, J Romie1, S Rowan18, A Rüdiger2, L Ruet4, P Russell1, K Ryan10, V Sandberg10, G H Sanders1,48, V Sannibale1, P Sarin4, B S Sathyaprakash8, P R Saulson23, R Savage10, A Sazonov22, R Schilling2, R Schofield15, B F Schutz7, P Schwinberg10, S M Scott33, S E Seader14, A C Searle33, B Sears1, D Sellers13, A S Sengupta8, P Shawhan1, D H Shoemaker4, A Sibley13, X Siemens3, D Sigg10, A M Sintes7,31, J Smith2, M R Smith1, O Spjeld13, K A Strain18, D M Strom15, A Stuver6, T Summerscales6, M Sung5, P J Sutton1, D B Tanner22, M Tarallo1, R Taylor1, K A Thorne6, K S Thorne37, K V Tokmakov12, C Torres26, C Torrie1, G Traylor13, W Tyler1, D Ugolini39, C Ungarelli21, M Vallisneri37, M van Putten4, S Vass1, A Vecchio21, J Veitch18, C Vorvick10, S P Vyachanin12, L Wallace1, H Ward18, R Ward1, K Watts13, D Webber1, U Weiland24, A Weinstein1, R Weiss4, S Wen5, K Wette33, J T Whelan34, S E Whitcomb1, B F Whiting22, S Wiley28, C Wilkinson10, P A Willems1, B Willke2,24, A Wilson1, W Winkler2, S Wise22, A G Wiseman3, G Woan18, D Woods3, R Wooley13, J Worden10, I Yakushin13, H Yamamoto1, S Yoshida40, M Zanolin4, L Zhang1, N Zotov41, M Zucker13 and J Zweizig1 (LIGO Scientific Collaboration)
Show affiliationsWe report on a search for gravitational-wave bursts in data from the three LIGO interferometric detectors during their third science run. The search targets sub-second 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 hrss ~ 10−20 Hz−1/2. No gravitational-wave signals were detected in the eight days of analysed data.
07.05.Kf Data analysis: algorithms and implementation; data management
95.85.Sz Gravitational radiation, magnetic fields, and other observations
Issue 8 (21 April 2006)
Received 14 October 2005, in final form 29 November 2005
Published 22 March 2006
B Abbott et al 2006 Class. Quantum Grav. 23 S29
M Barbieri et al 2009 New J. Phys. 11 093012
Dror Givon et al 2004 Nonlinearity 17 R55
M Lyatti et al 2009 Supercond. Sci. Technol. 22 114005
A Ney et al 2010 New J. Phys. 12 013020