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Astrophysically triggered searches for gravitational waves: status and prospects

B Abbott1, R Abbott1, R Adhikari1, P Ajith2, B Allen2,3, 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, 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 Chen10,27, 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 Danzmann2,9, G Davies28, D DeBra4, J Degallaix10, M Degree4, V Dergachev30, S Desai31, R DeSalvo1, S Dhurandhar32, M Díaz33, J Dickson34, 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 Fricke1,37, P Fritschel15, V V Frolov18, M Fyffe18, J Garofoli12, I Gholami10, J A Giaime5,18, 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, 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 Lück2,9, 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 Miller1,13, 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 Papa3,10, 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 Robertson1,13, 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 Schutz10,28, 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 Sintes10,51, B J J Slagmolen34, J Slutsky5, J R Smith21, M R Smith1, N D Smith15, K Somiya2,10, 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, 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 Willke2,9, 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, J Zweizig1 (The LIGO Scientific Collaboration), F Acernese56,57, M Alshourbagy58,59, P Amico60,61, F Antonucci62, S Aoudia63, P Astone62, S Avino56,64, L Baggio65, G Ballardin66, F Barone56,57, L Barsotti58,59, M Barsuglia67, Th S Bauer68, S Bigotta58,59, S Birindelli58,59, M A Bizouard67, C Boccara69, F Bondu63, L Bosi60, S Braccini58, C Bradaschia58, A Brillet63, V Brisson67, D Buskulic65, G Cagnoli70, E Calloni56,64, E Campagna70,71, F Carbognani66, F Cavalier67, R Cavalieri66, G Cella58, E Cesarini70,72, E Chassande-Mottin63, A-C Clapson67, F Cleva63, E Coccia73,74, C Corda58,59, A Corsi62, F Cottone60,61, J-P Coulon63, E Cuoco66, S D'Antonio73, A Dari60,61, V Dattilo66, M Davier67, R De Rosa56,64, M Del Prete58,75, L Di Fiore56, A Di Lieto58,59, M Di Paolo Emilio73,76, A Di Virgilio58, M Evans66, V Fafone73,74, I Ferrante58,59, F Fidecaro58,59, I Fiori66, R Flaminio77, J-D Fournier63, S Frasca62,78, F Frasconi58, L Gammaitoni60,61, F Garufi56,64, E Genin66, A Gennai58, A Giazotto66,58, L Giordano56,64, V Granata65, C Greverie63, D Grosjean65, G Guidi70,71, S Hamdani66, S Hebri66, H Heitmann63, P Hello67, D Huet66, S Kreckelbergh67, P La Penna66, M Laval63, N Leroy67, N Letendre65, B Lopez66, M Lorenzini70,72, V Loriette69, G Losurdo70, J-M Mackowski77, E Majorana62, C N Man63, M Mantovani59,75, F Marchesoni60,61, F Marion65, J Marque66, F Martelli70,71, A Masserot65, F Menzinger66, L Milano56,64, Y Minenkov73, C Moins66, J Moreau69, N Morgado77, S Mosca56,64, B Mours65, I Neri60,61, F Nocera66, G Pagliaroli73, C Palomba62, F Paoletti66,58, S Pardi56,64, A Pasqualetti66, R Passaquieti58,59, D Passuello58, F Piergiovanni70,71, L Pinard77, R Poggiani58,59, M Punturo60, P Puppo62, P Rapagnani62,78, T Regimbau63, A Remillieux77, F Ricci62,78, I Ricciardi56,64, A Rocchi73, L Rolland65, R Romano56,57, P Ruggi66, G Russo56,64, S Solimeno56,64, A Spallicci63, B L Swinkels66, M Tarallo58,59, R Terenzi73, A Toncelli58,59, M Tonelli58,59, E Tournefier65, F Travasso60,61, G Vajente79,59, J F J van den Brand68,80, S van der Putten68, D Verkindt65, F Vetrano70,71, A Viceré70,71, J-Y Vinet63, H Vocca60 and M Yvert65 (The Virgo Collaboration)

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In gravitational-wave detection, special emphasis is put onto searches that focus on cosmic events detected by other types of astrophysical observatories. The astrophysical triggers, e.g. from γ-ray and x-ray satellites, optical telescopes and neutrino observatories, provide a trigger time for analyzing gravitational-wave data coincident with the event. In certain cases the expected frequency range, source energetics, directional and progenitor information are also available. Beyond allowing the recognition of gravitational waveforms with amplitudes closer to the noise floor of the detector, these triggered searches should also lead to rich science results even before the onset of Advanced LIGO. In this paper we provide a broad review of LIGO's astrophysically triggered searches and the sources they target.


PACS

04.80.Nn Gravitational wave detectors and experiments

95.55.Ym Gravitational radiation detectors; mass spectrometers; and other instrumentation and techniques

MSC

85A04 General

83C35 Gravitational waves

Subjects

Instrumentation and measurement

Gravitation and cosmology

Astrophysics and astroparticles

Dates

Issue 11 (7 June 2008)

Received 10 January 2008, in final form 25 February 2008

Published 15 May 2008



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