Search for gravitational-wave inspiral signals associated with short gamma-ray bursts during LIGO’s fifth and VIRGO’s first science run
Year: 2010
Authors: Abadie J., Abbott B. P., Abbott R., Accadia T., Acernese F., Adhikari R., Ajith P., Allen B., Allen G., Amador Ceron E., Amin R. S., Anderson S. B., Anderson W. G., Antonucci F., Aoudia S., Arain M. A., Araya M., Arun K. G., Aso Y., Aston S., Astone P., Aufmuth P., Aulbert C., Babak S., Baker P., Ballardin G., Ballmer S., Barker D., Barone F., Barr B., Barriga P. Barsotti L., Barsuglia M., Barton M.A., Bartos I., Bassiri R., Bastarrika M., Bauer Th. S., Behnke B., Beker M.G., Belletoile A., Benacquista M., Betzwieser J., Beyersdorf P.T., Bigotta S., Bilenko I.A., Billingsley G ., Birindelli S., Biswas R., Bizouard M.A., Black E., Blackburn J.K., Blackburn L., Blair D., Bland B., Blom M., Boccara C., Bock O., Bodiya T. P., Bondarescu R., Bondu F., Bonelli L., Bonnand R., Bork R., Born M., Bose S., Bosi L., Braccini S., Bradaschia C., Brady P.R., Braginsky V.B., Brau J.E., Breyer J., Bridges D.O., Brillet A., Brinkmann M., Brisson V., Britzger M., Brooks A.F., Brown D.A., Budzynski R., Bulik T., Bullington A., Bulten H.J., Buonanno A., Burguet-Castell J., Burmeister O., Buskulic D., Buy C., Byer R.L., Cadonati L., Cagnoli G., Cain J., Calloni E., Camp J.B., Campagna E., Cannizzo J., Cannon K.C., Canuel B., Cao J., Capano C.D., Carbognani F., Cardenas L., Caudill S., Cavaglia M., Cavalier F., Cavalieri R., Cella G., Cepeda C., Cesarini E., Chalermsongsak T., Chalkley E., Charlton P., Chassande-Mottin E., Chatterji S., Chelkowski S., Chen Y., Chincarini A., Christensen N., Chua S.S.Y., Chung C.T.Y., Clark D., Clark J., Clayton J.H., Cleva F., Coccia E., Colacino C.N., Colas J., Colla A., Colombini M., Conte R., Cook D., Corbitt T.R.C., Cornish N., Corsi A., Coulon J.P., Coward D., Coyne D.C., Creighton J.D.E., Creighton T.D., Cruise A. M., Culter R.M., Cumming A., Cunningham L., Cuoco E., Dahl K., Danilishin S.L., D’Antonio S., Danzmann K., Dattilo V., Daudert B., Davier M., Davies G., Daw E.J., Day R., Dayanga T., De Rosa R., DeBra D., Degallaix J., del Prete M., Dergachev V., DeSalvo R., Dhurandhar S., Di Fiore L., Di Lieto A., Emilio M.D., Di Virgilio A., Diaz M., Dietz A., Donovan F., Dooley K.L., Doomes E.E., Drago M., Drever R.W.P., Driggers J., Dueck J., Duke I., Dumas J.C., Edgar M., Edwards M., Effler A., Ehrens P., Etzel T., Evans M., Evans T., Fafone V., Fairhurst S., Faltas Y., Fan Y., Fazi D., Fehrmann H., Ferrante I., Fidecaro F., Finn L.S., Fiori I., Flaminio R. Flasch K., Foley S., Forrest C., Fotopoulos N., Fournier J.D., Franc J., Frasca S., Frasconi F., Frede M., Frei M., Frei Z., Freise A., Frey R., Fricke T.T., Friedrich D., Fritschel P., Frolov V.V., Fulda P., Fyffe M., Galimberti M., Gammaitoni L., Garofoli J.A. Garufi F., Gemme G., Genin E., Gennai A., Ghosh S., Giaime J.A., Giampanis S., Giardina K.D., Giazotto A., Goetz E., Goggin L.M., Gonzalez G., Gossler S., Gouaty R., Granata M., Grant A., Gras S., Gray C., Greenhalgh R. J. S., Gretarsson A. M., Greverie C., Grosso R., Grote H., Grunewald S., Guidi G.M., Gustafson E.K., Gustafson R., Hage B., Hallam J.M., Hammer D., Hammond G.D., Hanna C., Hanson J., Harms J., Harry G. M., Harry I.W., Harstad E.D., Haughian K., Hayama K., Hayler T., Heefner J., Heitmann H., Hello P., Heng I.S., Heptonstall A., Hewitson M., Hild S., Hirose E., Hoak D., Hodge K.A., Holt K., Hosken D.J., Hough J., Howell E., Hoyland D., Huet D., Hughey B., Husa S., Huttner S.H., Ingram D.R., Isogai T., Ivanov A., Jaranowski P., Johnson W.W., Jones D.I., Jones G., Jones R., Ju L., Kalmus P., Kalogera V., Kandhasamy S., Kanner J., Katsavounidis E., Kawabe K., Kawamura S., Kawazoe F., Kells W., Keppel D.G., Khalaidovski A., Khalili F.Y., Khan R., Khazanov E., Kim H., King P.J., Kissel J.S., Klimenko S., Kokeyama K., Kondrashov V., Kopparapu R.; Koranda S., Kowalska I., Kozak D., Kringel V., Krishnan B., Krolak A., Kuehn G., Kullman J., Kumar R., Kwee P., Lam P. K., Landry M., Lang M., Lantz B., Lastzka N., Lazzarini A., Leaci P., Lei M., Leindecker N., Leonor I., Leroy N., Letendre N., Li T.G.F., Lin H., Lindquist P.E., Littenberg T.B., Lockerbie N.A., Lodhia D., Lorenzini M., Loriette V., Lormand M., Losurdo G., Lu P., Lubinski M., Lucianetti A., Lueck H., Lundgren A., Machenschalk B., MacInnis M., Mageswaran M., Mailand K., Majorana E. Mak C., Maksimovic I., Man N., Mandel I., Mandic V., Mantovani M., Marchesoni F., Marion F., Marka S., Marka Z., Markosyan A., Markowitz J., Maros E., Marque J., Martelli F., Martin I.W., Martin R.M., Marx J.N., Mason K., Masserot A., Matichard F., Matone L., Matzner R.A., Mavalvala N., McCarthy R., McClelland D.E., McGuire S.C., McIntyre G., McKechan D.J.A., Mehmet M., Melatos A., Melissinos A., Mendell G., Menendez D.F., Mercer R.A., Merill L., Meshkov S., Messenger C., Meyer M.S., Miao H., Michel C., Milano L., Miller J., Minenkov Y., Mino Y., Mitra S., Mitrofanov V.P., Mitselmakher G., Mittleman R., Miyakawa O., Moe B., Mohan M., Mohanty S.D., Mohapatra S.R.P., Moreau J., Moreno G., Morgado N., Morgia A., Mors K., Mosca S., Moscatelli V., Mossavi K., Mours B., MowLowry C., Mueller G., Mukherjee S., Mullavey A., Mueller-Ebhardt H., Munch J., Murray P.G., Nash T., Nawrodt R., Nelson J., Neri I., Newton G., Nishida E., Nishizawa A., Nocera F., Ochsner E., O’Dell J., Ogin G.H., Oldenburg R., O’Reilly B., O’Shaughnessy R., Ottaway D.J., Ottens R.S., Overmier H., Owen B.J., Page A., Pagliaroli G., Palomba C., Pan Y., Pankow C., Paoletti F., Papa M.A., Pardi S., Parisi M., Pasqualetti A., Passaquieti R., Passuello D., Patel P., Pathak D., Pedraza M., Pekowsky L., Penn S., Peralta C., Perreca A., Persichetti G., Pichot M., Pickenpack M., Piergiovanni F., Pietka M., Pinard L., Pinto I. M., Pitkin M., Pletsch H. J., Plissi M. V., Poggiani R, Postiglione F., Prato M., Predoi V., Principe M., Prix R., Prodi G. A., Prokhorov L., Puncken O., Punturo M., Puppo P., Quetschke V., Raab F. J., Rabeling D. S., Radkins H., Raffai P., Raics Z., Rakhmanov M., Rapagnani P., Raymond V., Re V., Reed C. M., Reed T., Regimbau T., Rehbein H., Reid S., Reitze D. H., Ricci F., Riesen R., Riles K., Roberts P., Robertson N.A., Robinet F., Robinson C., Robinson E. L., Rocchi A., Roddy S., Rover C., Rolland L., Rollins J., Romano J. D., Romano R., Romie J. H., Rosinska D., Rowan S., Rudiger A., Ruggi P., Ryan K., Sakata S., Salemi F., Sammut L., Sancho de la Jordana L., Sandberg V., Sannibale V., Santamaria L., Santostasi G., Saraf S., Sarin P., Sassolas B., Sathyaprakash B. S., Sato S., Satterthwaite M., Saulson P. R., Savage R., Schilling R., Schnabel R., Schofield R., Schulz B., Schutz B. F., Schwinberg P., Scott J., Scott S. M., Searle A. C., Seifert F., Sellers D., Sengupta A. S., Sentenac D., Sergeev A., Shapiro B., Shawhan P., Shoemaker D. H., Sibley A., Siemens X., Sigg D., Sintes A. M., Skelton G., Slagmolen B. J. J., Slutsky J., Smith J. R., Smith M. R., Smith N. D., Somiya K., Sorazu B., Stein A. J., Stein L. C., Steplewski S., Stochino A., Stone R., Strain K. A., Strigin S., Stroeer A., Sturani R., Stuver A. L., Summerscales T.Z., Sung M., Susmithan S., Sutton P. J., Swinkels B., Szokoly G. P., Talukder D., Tanner D. B., Tarabrin S. P., Taylor J. R., Taylor R., Thorne K. A., Thorne K. S., Thuering A., Titsler C., Tokmakov K. V., Toncelli A., Tonelli M., Torres C., Torrie C. I., Tournefier E., Travasso F., Traylor G.., Trias M., Trummer J., Turner L., Ugolini D., Urbanek K., Vahlbruch H., Vajente G., Vallisneri M., van den Brand J. F. J., Van Den Broeck C., van der Putten S., van der Sluys M. V., Vass S., Vaulin R., Vavoulidis M., Vecchio A., Vedovato G., van Veggel A. A., Veitch J., Veitch P. J., Veltkamp C., Verkindt D., Vetrano F., Vicere A., Villar A., Vinet J. -Y., Vocca H., Vorvick C., Vyachanin S.P., Waldman S.J., Wallace L., Wanner A., Ward R.L., Was M., Wei P., Weinert M., Weinstein A. J., Weiss R., Wen L., Wen S., Wessels P., West M., Westphal T., Wette K., Whelan J.T., Whitcomb S.E., Whiting B. F., Wilkinson C., Willems P. A., Williams H. R., Williams L., Willke B., Wilmut I., Winkelmann L., Winkler W., Wipf C. C., Wiseman A. G., Woan G., Wooley R., Worden J., Yakushin I., Yamamoto H., Yamamoto K., Yeaton-Massey D., Yoshida S., Yu P.P., Yvert M., Zanolin M., Zhang L., Zhang Z., Zhao C., Zotov N., Zucker M. E., Zweizig J.
Autors Affiliation: LIGO CALTECH, Pasadena, CA 91125 USA; Univ Savoie, LAPP, CNRS, IN2P3, F-74941 Annecy Le Vieux, France; Complesso Univ Monte St Angelo, Ist Nazl Fis Nucl, Sez Napoli, I-80126 Naples, Italy; Univ Salerno, I-84084 Salerno, Italy; Max Planck Inst Gravitat Phys, Albert Einstein Inst, D-30167 Hannover, Germany; Univ Wisconsin, Milwaukee, WI 53201 USA; Stanford Univ, Stanford, CA 94305 USA; Louisiana State Univ, Baton Rouge, LA 70803 USA; INFN, Sez Roma, I-00185 Rome, Italy; Univ Nice Sophia Antipolis, CNRS, Observ Cote Azur, F-06304 Nice, France; Univ Florida, Gainesville, FL 32611 USA; Univ Paris 11, LAL, CNRS, IN2P3, F-91898 Orsay, France; Univ Birmingham, Birmingham B15 2TT, W Midlands, England; Leibniz Univ Hannover, D-30167 Hannover, Germany; Max Planck Inst Gravitat Phys, Albert Einstein Inst, D-14476 Golm, Germany; Montana State Univ, Bozeman, MT 59717 USA; EGO, I-56021 Cascina, Pi, Italy; LIGO Hanford Observ, Richland, WA 99352 USA; Univ Glasgow, Glasgow G12 8QQ, Lanark, Scotland; Univ Western Australia, Crawley, WA 6009, Australia; LIGO MIT, Cambridge, MA 02139 USA; Univ Denis Diderot Paris 7, CNRS, IN2P3, Observ Paris,DSM,IRFU,CEA,UMR7164, Paris, France; Columbia Univ, New York, NY 10027 USA; Nikhef, Natl Inst Subatom Phys, NL-1009 DB Amsterdam, Netherlands; Univ Texas Brownsville & Texas Southmost Coll, Brownsville, TX 78520 USA; San Jose State Univ, San Jose, CA 95192 USA; INFN, Sez Pisa, I-56127 Pisa, Italy; Univ Pisa, I-56127 Pisa, Italy; Moscow MV Lomonosov State Univ, Moscow 119992, Russia; CNRS, ESPCI, F-75005 Paris, France; Penn State Univ, University Pk, PA 16802 USA; Univ Rennes 1, Inst Phys Rennes, CNRS, F-35042 Rennes, France; CNRS, LMA, IN2P3, F-69622 Lyon, France; Washington State Univ, Pullman, WA 99164 USA; INFN, Sez Perugia, I-6123 Perugia, Italy; Univ Oregon, Eugene, OR 97403 USA; Livingston Observ, LIGO, Livingston, LA 70754 USA; Syracuse Univ, Syracuse, NY 13244 USA; Warsaw Univ, PL-00681 Warsaw, Poland; Warsaw Univ, Astro Obs, PL-00478 Warsaw, Poland; CAMK PAN, PL-00716 Warsaw, Poland; Vrije Univ Amsterdam, NL-1081 HV Amsterdam, Netherlands; Univ Maryland, College Pk, MD 20742 USA; Univ Massachusetts, Amherst, MA 01003 USA; INFN, Sez Firenze, I-50019 Sesto Fiorentino, Italy; Univ Mississippi, University, MS 38677 USA; Univ Naples Federico II, I-80126 Naples, Italy; NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA; Univ Urbino Carlo Bo, I-61029 Urbino, Italy; Charles Sturt Univ, Wagga Wagga, NSW 2678, Australia; CALTECH, CaRT, Pasadena, CA 91125 USA; INFN, Sez Genova, I-16146 Genoa, Italy; Carleton Coll, Northfield, MN 55057 USA; Australian Natl Univ, Canberra, ACT 0200, Australia; Univ Melbourne, Parkville, Vic 3010, Australia; Cardiff Univ, Cardiff CF24 3AA, S Glam, Wales; INFN, Sez Roma Tor Vergata, I-00133 Rome, Italy; Univ Roma Tor Vergata, I-00133 Rome, Italy; Univ Roma La Sapienza, I-00185 Rome, Italy; Univ Sheffield, Sheffield S10 2TN, S Yorkshire, England; Univ Siena, I-53100 Siena, Italy; Univ Michigan, Ann Arbor, MI 48109 USA; Interuniv Ctr Astron & Astrophys, Pune 411007, Maharashtra, India; Univ Aquila, I-67100 Laquila, Italy; INAF, IFSI, I-00133 Rome, Italy; INFN, Sez Padova, I-35131 Padua, Italy; Univ Padua, I-35131 Padua, Italy; Univ Rochester, Rochester, NY 14627 USA; Univ Texas Austin, Austin, TX 78712 USA; Eutvus Univ, ELTE, H-1053 Budapest, Hungary; Univ Perugia, I-6123 Perugia, Italy; Rutherford Appleton Lab, HSIC, Didcot OX11 0QX, Oxon, England; Embry Riddle Aeronaut Univ, Prescott, AZ 86301 USA; Univ Minnesota, Minneapolis, MN 55455 USA; Univ Adelaide, Adelaide, SA 5005, Australia; Univ Illes Balears, E-07122 Palma de Mallorca, Spain; Bialystok Univ, PL-15424 Bialystok, Poland; Univ Southampton, Southampton SO17 1BJ, Hants, England; Northwestern Univ, Evanston, IL 60208 USA; Natl Astron Observ Japan, Tokyo 1818588, Japan; Inst Appl Phys, Nizhnii Novgorod 603950, Russia; IM PAN, PL-00956 Warsaw, Poland; IPJ, PL-05400 Otwock, Poland; Univ Strathclyde, Glasgow G1 1XQ, Lanark, Scotland; Hobart & William Smith Coll, Geneva, NY 14456 USA; Univ Sannio Benevento, I-82100 Benevento, Italy; Grp Collegato Trento, INFN, I-38050 Trento, Italy; Univ Trent, I-38050 Trento, Italy; Louisiana Tech Univ, Ruston, LA 71272 USA; Andrews Univ, Berrien Springs, MI 49104 USA; Inst Astron, PL-65265 Zielona Gora, Poland; McNeese State Univ, Lake Charles, LA 70609 USA; Sonoma State Univ, Rohnert Pk, CA 94928 USA; Trinity Univ, San Antonio, TX 78212 USA; Rochester Inst Technol, Rochester, NY 14623 USA; SE Louisiana Univ, Hammond, LA 70402 USA; CALTECH, Pasadena, CA 91125 USA
Abstract: Progenitor scenarios for short gamma-ray bursts (short GRBs) include coalescenses of two neutron stars or a neutron star and black hole, which would necessarily be accompanied by the emission of strong gravitational waves. We present a search for these known gravitational-wave signatures in temporal and directional coincidence with 22 GRBs that had sufficient gravitational-wave data available in multiple instruments during LIGO\’s fifth science run, S5, and Virgo’s first science run, VSR1. We find no statistically significant gravitational-wave candidates within a [−5, +1) s window around the trigger time of any GRB. Using the Wilcoxon–Mann–Whitney U-test, we find no evidence for an excess of weak gravitational-wave signals in our sample of GRBs. We exclude neutron star–black hole progenitors to a median 90% confidence exclusion distance of 6.7 Mpc.
Journal/Review: ASTROPHYSICAL JOURNAL
Volume: 715 (2) Pages from: 1453 to: 1461
More Information: We are indebted to the observers of the electromagnetic events and the GCN for providing us with valuable data. The authors gratefully acknowledge the support of the United States National Science Foundation for the construction and operation of the LIGO Laboratory, the Science and Technology Facilities 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, and the Italian Istituto Nazionale di Fisica Nucleare and the French Centre National de la Recherche Scientifique for the construction and operation of the Virgo detector. The authors also gratefully acknowledge research support by these agencies and by the Australian Research Council, the Council of Scientific and Industrial Research of India, the Istituto Nazionale di Fisica Nucleare of Italy, the Spanish Ministerio de Educacion y Ciencia, the Conselleria d\’Economia Hisenda i Innovacio of the Govern de les Illes Balears, the Foundation for Fundamental Research on Matter supported by the Netherlands Organisation for Scientific Research, the Royal Society, the Scottish Funding Council, the Scottish Universities Physics Alliance, The National Aeronautics and Space Administration, the Carnegie Trust, the Leverhulme Trust, the David and Lucile Packard Foundation, the Research Corporation, and the Alfred P. Sloan Foundation.KeyWords: binaries: close; gamma-ray burst: general; gravitational waves; Virgo; LIGODOI: 10.1088/0004-637X/715/2/1453ImpactFactor: 6.063Citations: 86data from “WEB OF SCIENCE” (of Thomson Reuters) are update at: 2024-11-10References taken from IsiWeb of Knowledge: (subscribers only)Connecting to view paper tab on IsiWeb: Click hereConnecting to view citations from IsiWeb: Click here
