First joint search for gravitational-wave bursts in LIGO and GEO 600 data

doi:10.1088/0264-9381/25/24/245008

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Classical and Quantum Gravity

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Classical and Quantum Gravity Volume 25 Number 24 Create an alert RSS this journal

B Abbott et al 2008 Class. Quantum Grav. 25 245008 doi:10.1088/0264-9381/25/24/245008

First joint search for gravitational-wave bursts in LIGO and GEO 600 data

B Abbott¹, R Abbott¹, R Adhikari¹, P Ajith², B Allen^2,3, G Allen⁴, R Amin⁵, S B Anderson¹, W G Anderson³, M A Arain⁶, M Araya¹, H Armandula¹, P Armor³, Y Aso⁷, S Aston⁸, P Aufmuth⁹, C Aulbert², S Babak¹⁰, S Ballmer¹, H Bantilan¹¹, B C Barish¹, C Barker¹², D Barker¹², B Barr¹³, P Barriga¹⁴, M A Barton¹³, I Bartos⁷, M Bastarrika¹³, K Bayer¹⁵, J Betzwieser¹, P T Beyersdorf¹⁶, I A Bilenko¹⁷, G Billingsley¹, R Biswas³, E Black¹, K Blackburn¹, L Blackburn¹⁵, D Blair¹⁴, B Bland¹², T P Bodiya¹⁵, L Bogue¹⁸, R Bork¹, V Boschi¹, S Bose¹⁹, P R Brady³, V B Braginsky¹⁷, J E Brau²⁰, M Brinkmann², A Brooks¹, D A Brown²¹, G Brunet¹⁵, A Bullington⁴, A Buonanno²², O Burmeister², R L Byer⁴, L Cadonati²³, G Cagnoli¹³, J B Camp²⁴, J Cannizzo²⁴, K Cannon¹, J Cao¹⁵, L Cardenas¹, T Casebolt⁴, G Castaldi²⁵, C Cepeda¹, E Chalkley¹³, P Charlton²⁶, S Chatterji¹, S Chelkowski⁸, Y Chen^10,27, N Christensen¹¹, D Clark⁴, J Clark¹³, T Cokelaer²⁸, R Conte²⁹, D Cook¹², T Corbitt¹⁵, D Coyne¹, J D E Creighton³, A Cumming¹³, L Cunningham¹³, R M Cutler⁸, J Dalrymple²¹, K Danzmann^2,9, G Davies²⁸, D DeBra⁴, J Degallaix¹⁰, M Degree⁴, V Dergachev³⁰, S Desai³¹, R DeSalvo¹, S Dhurandhar³², M Díaz³³, J Dickson³⁴, A Di Credico²¹, A Dietz²⁸, F Donovan¹⁵, K L Dooley⁶, E E Doomes³⁵, R W P Drever³⁶, I Duke¹⁵, J-C Dumas¹⁴, R J Dupuis¹, J G Dwyer⁷, C Echols¹, A Effler¹², P Ehrens¹, E Espinoza¹, T Etzel¹, T Evans¹⁸, S Fairhurst²⁸, Y Fan¹⁴, D Fazi¹, H Fehrmann², M M Fejer⁴, L S Finn³¹, K Flasch³, N Fotopoulos³, A Freise⁸, R Frey²⁰, T Fricke^1,37, P Fritschel¹⁵, V V Frolov¹⁸, M Fyffe¹⁸, J Garofoli¹², I Gholami¹⁰, J A Giaime^5,18, S Giampanis³⁷, K D Giardina¹⁸, K Goda¹⁵, E Goetz³⁰, L Goggin¹, G González⁵, S Gossler², R Gouaty⁵, A Grant¹³, S Gras¹⁴, C Gray¹², M Gray³⁴, R J S Greenhalgh³⁸, A M Gretarsson³⁹, F Grimaldi¹⁵, R Grosso³³, H Grote², S Grunewald¹⁰, M Guenther¹², E K Gustafson¹, R Gustafson³⁰, B Hage⁹, J M Hallam⁸, D Hammer³, C Hanna⁵, J Hanson¹⁸, J Harms², G Harry¹⁵, E Harstad²⁰, K Hayama³³, T Hayler³⁸, J Heefner¹, I S Heng¹³, M Hennessy⁴, A Heptonstall¹³, M Hewitson², S Hild⁸, E Hirose²¹, D Hoak¹⁸, D Hosken⁴⁰, J Hough¹³, B Hughey¹⁵, S H Huttner¹³, D Ingram¹², M Ito²⁰, A Ivanov¹, B Johnson¹², W W Johnson⁵, D I Jones⁴¹, G Jones²⁸, R Jones¹³, L Ju¹⁴, P Kalmus⁷, V Kalogera⁴², S Kamat⁷, J Kanner²², D Kasprzyk⁸, E Katsavounidis¹⁵, K Kawabe¹², S Kawamura⁴³, F Kawazoe⁴³, W Kells¹, D G Keppel¹, F Ya Khalili¹⁷, R Khan⁷, E Khazanov⁴⁴, C Kim⁴², P King¹, J S Kissel⁵, S Klimenko⁶, K Kokeyama⁴³, V Kondrashov¹, R K Kopparapu³¹, D Kozak¹, I Kozhevatov⁴⁴, B Krishnan¹⁰, P Kwee⁹, P K Lam³⁴, M Landry¹², M M Lang³¹, B Lantz⁴, A Lazzarini¹, M Lei¹, N Leindecker⁴, V Leonhardt⁴³, I Leonor²⁰, K Libbrecht¹, H Lin⁶, P Lindquist¹, N A Lockerbie⁴⁵, D Lodhia⁸, M Lormand¹⁸, P Lu⁴, M Lubinski¹², A Lucianetti⁶, H Lück^2,9, B Machenschalk², M MacInnis¹⁵, M Mageswaran¹, K Mailand¹, V Mandic⁴⁶, S Márka⁷, Z Márka⁷, A Markosyan⁴, J Markowitz¹⁵, E Maros¹, I Martin¹³, R M Martin⁶, J N Marx¹, K Mason¹⁵, F Matichard⁵, L Matone⁷, R Matzner⁴⁷, N Mavalvala¹⁵, R McCarthy¹², D E McClelland³⁴, S C McGuire³⁵, M McHugh⁴⁸, G McIntyre¹, G McIvor⁴⁷, D McKechan²⁸, K McKenzie³⁴, T Meier⁹, A Melissinos³⁷, G Mendell¹², R A Mercer⁶, S Meshkov¹, C J Messenger², D Meyers¹, J Miller^1,13, J Minelli³¹, S Mitra³², V P Mitrofanov¹⁷, G Mitselmakher⁶, R Mittleman¹⁵, O Miyakawa¹, B Moe³, S Mohanty³³, G Moreno¹², K Mossavi², C MowLowry³⁴, G Mueller⁶, S Mukherjee³³, H Mukhopadhyay³², H Müller-Ebhardt², J Munch⁴⁰, P Murray¹³, E Myers¹², J Myers¹², T Nash¹, J Nelson¹³, G Newton¹³, A Nishizawa⁴³, K Numata²⁴, J O'Dell³⁸, G Ogin¹, B O'Reilly¹⁸, R O'Shaughnessy³¹, D J Ottaway¹⁵, R S Ottens⁶, H Overmier¹⁸, B J Owen³¹, Y Pan²², C Pankow⁶, M A Papa^3,10, V Parameshwaraiah¹², P Patel¹, M Pedraza¹, S Penn⁴⁹, A Perreca⁸, T Petrie³¹, I M Pinto²⁵, M Pitkin¹³, H J Pletsch², M V Plissi¹³, F Postiglione²⁹, M Principe²⁵, R Prix², V Quetschke⁶, F Raab¹², D S Rabeling³⁴, H Radkins¹², N Rainer², M Rakhmanov⁵⁰, M Ramsunder³¹, H Rehbein², S Reid¹³, D H Reitze⁶, R Riesen¹⁸, K Riles³⁰, B Rivera¹², N A Robertson^1,13, C Robinson²⁸, E L Robinson⁸, S Roddy¹⁸, A Rodriguez⁵, A M Rogan¹⁹, J Rollins⁷, J D Romano³³, J Romie¹⁸, R Route⁴, S Rowan¹³, A Rüdiger², L Ruet¹⁵, P Russell¹, K Ryan¹², S Sakata⁴³, M Samidi¹, L Sancho de la Jordana⁵¹, V Sandberg¹², V Sannibale¹, S Saraf⁵², P Sarin¹⁵, B S Sathyaprakash²⁸, S Sato⁴³, P R Saulson²¹, R Savage¹², P Savov²⁷, S W Schediwy¹⁴, R Schilling², R Schnabel², R Schofield²⁰, B F Schutz^10,28, P Schwinberg¹², S M Scott³⁴, A C Searle³⁴, B Sears¹, F Seifert², D Sellers¹⁸, A S Sengupta¹, P Shawhan²², D H Shoemaker¹⁵, A Sibley¹⁸, X Siemens³, D Sigg¹², S Sinha⁴, A M Sintes^10,51, B J J Slagmolen³⁴, J Slutsky⁵, J R Smith²¹, M R Smith¹, N D Smith¹⁵, K Somiya^2,10, B Sorazu¹³, L C Stein¹⁵, A Stochino¹, R Stone³³, K A Strain¹³, D M Strom²⁰, A Stuver¹⁸, T Z Summerscales⁵³, K-X Sun⁴, M Sung⁵, P J Sutton²⁸, H Takahashi¹⁰, D B Tanner⁶, R Taylor¹, R Taylor¹³, J Thacker¹⁸, K A Thorne³¹, K S Thorne²⁷, A Thüring⁹, M Tinto¹, K V Tokmakov¹³, C Torres¹⁸, C Torrie¹³, G Traylor¹⁸, M Trias⁵¹, W Tyler¹, D Ugolini⁵⁴, J Ulmen⁴, K Urbanek⁴, H Vahlbruch⁹, C Van Den Broeck²⁸, M van der Sluys⁴², S Vass¹, R Vaulin³, A Vecchio⁸, J Veitch⁸, P Veitch⁴⁰, A Villar¹, C Vorvick¹², S P Vyachanin¹⁷, S J Waldman¹, L Wallace¹, H Ward¹³, R Ward¹, M Weinert², A Weinstein¹, R Weiss¹⁵, S Wen⁵, K Wette³⁴, J T Whelan¹⁰, S E Whitcomb¹, B F Whiting⁶, C Wilkinson¹², P A Willems¹, H R Williams³¹, L Williams⁶, B Willke^2,9, I Wilmut³⁸, W Winkler², C C Wipf¹⁵, A G Wiseman³, G Woan¹³, R Wooley¹⁸, J Worden¹², W Wu⁶, I Yakushin¹⁸, H Yamamoto¹, Z Yan¹⁴, S Yoshida⁵⁰, M Zanolin³⁹, J Zhang³⁰, L Zhang¹, C Zhao¹⁴, N Zotov⁵⁵, M Zucker¹⁵ and J Zweizig¹ (LIGO Scientific Collaboration)

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i.heng@physics.gla.ac.uk

¹ LIGO—California Institute of Technology, Pasadena, CA 91125, USA
² Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
³ University of Wisconsin-Milwaukee, Milwaukee, WI 53201, USA
⁴ Stanford University, Stanford, CA 94305, USA
⁵ Louisiana State University, Baton Rouge, LA 70803, USA
⁶ University of Florida, Gainesville, FL 32611, USA
⁷ Columbia University, New York, NY 10027, USA
⁸ University of Birmingham, Birmingham, B15 2TT, UK
⁹ Leibniz Universität Hannover, D-30167 Hannover, Germany
¹⁰ Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-14476 Golm, Germany
¹¹ Carleton College, Northfield, MN 55057, USA
¹² LIGO Hanford Observatory, Richland, WA 99352, USA
¹³ University of Glasgow, Glasgow, G12 8QQ, UK
¹⁴ University of Western Australia, Crawley, WA 6009, Australia
¹⁵ LIGO—Massachusetts Institute of Technology, Cambridge, MA 02139, USA
¹⁶ San Jose State University, San Jose, CA 95192, USA
¹⁷ Moscow State University, Moscow, 119992, Russia
¹⁸ LIGO Livingston Observatory, Livingston, LA 70754, USA
¹⁹ Washington State University, Pullman, WA 99164, USA
²⁰ University of Oregon, Eugene, OR 97403, USA
²¹ Syracuse University, Syracuse, NY 13244, USA
²² University of Maryland, College Park, MD 20742, USA
²³ University of Massachusetts, Amherst, MA 01003, USA
²⁴ NASA/Goddard Space Flight Center, Greenbelt, MD 20771, USA
²⁵ University of Sannio at Benevento, I-82100 Benevento, Italy
²⁶ Charles Sturt University, Wagga Wagga, NSW 2678, Australia
²⁷ Caltech-CaRT, Pasadena, CA 91125, USA
²⁸ Cardiff University, Cardiff, CF24 3AA, UK
²⁹ University of Salerno, 84084 Fisciano (Salerno), Italy
³⁰ University of Michigan, Ann Arbor, MI 48109, USA
³¹ The Pennsylvania State University, University Park, PA 16802, USA
³² Inter-University Centre for Astronomy and Astrophysics, Pune - 411007, India
³³ The University of Texas at Brownsville and Texas Southmost College, Brownsville, TX 78520, USA
³⁴ Australian National University, Canberra, 0200, Australia
³⁵ Southern University and A\&M College, Baton Rouge, LA 70813, USA
³⁶ California Institute of Technology, Pasadena, CA 91125, USA
³⁷ University of Rochester, Rochester, NY 14627, USA
³⁸ Rutherford Appleton Laboratory, Chilton, Didcot, Oxon OX11 0QX, UK
³⁹ Embry-Riddle Aeronautical University, Prescott, AZ 86301, USA
⁴⁰ University of Adelaide, Adelaide, SA 5005, Australia
⁴¹ University of Southampton, Southampton, SO17 1BJ, UK
⁴² Northwestern University, Evanston, IL 60208, USA
⁴³ National Astronomical Observatory of Japan, Tokyo 181-8588, Japan
⁴⁴ Institute of Applied Physics, Nizhny Novgorod, 603950, Russia
⁴⁵ University of Strathclyde, Glasgow, G1 1XQ, UK
⁴⁶ University of Minnesota, Minneapolis, MN 55455, USA
⁴⁷ The University of Texas at Austin, Austin, TX 78712, USA
⁴⁸ Loyola University, New Orleans, LA 70118, USA
⁴⁹ Hobart and William Smith Colleges, Geneva, NY 14456, USA
⁵⁰ Southeastern Louisiana University, Hammond, LA 70402, USA
⁵¹ Universitat de les Illes Balears, E-07122 Palma de Mallorca, Spain
⁵² Sonoma State University, Rohnert Park, CA 94928, USA
⁵³ Andrews University, Berrien Springs, MI 49104, USA
⁵⁴ Trinity University, San Antonio, TX 78212, USA
⁵⁵ Louisiana Tech University, Ruston, LA 71272, USA

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Abstract References Cited By

We present the results of the first joint search for gravitational-wave bursts by the LIGO and GEO 600 detectors. We search for bursts with characteristic central frequencies in the band 768–2048 Hz in the data acquired between 22 February and 23 March, 2005 (fourth LSC Science Run–S4). We discuss the inclusion of the GEO 600 data in the Waveburst–CorrPower pipeline that first searches for coincident excess power events without taking into account differences in the antenna responses or strain sensitivities of the various detectors. We compare the performance of this pipeline to that of the coherent Waveburst pipeline based on the maximum likelihood statistic. This likelihood statistic is derived from a coherent sum of the detector data streams that takes into account the antenna patterns and sensitivities of the different detectors in the network. We find that the coherent Waveburst pipeline is sensitive to signals of amplitude 30–50% smaller than the Waveburst–CorrPower pipeline. We perform a search for gravitational-wave bursts using both pipelines and find no detection candidates in the S4 data set when all four instruments were operating stably.

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