All-sky search for gravitational-wave bursts in the second joint LIGO-Virgo run

Year: 2012

Authors: Abadie J., Abbott B. P., Abbott R., Abbott T. D., Abernathy M., Accadia T., Acernese F., Adams C., Adhikari R., Affeldt C., Agathos M., Agatsuma K., Ajith P., Allen B., Amador Ceron E., Amariutei D., Anderson S. B., Anderson W. G., Arai K., Arain M. A., Araya M. C., Aston S. M., Astone P., Atkinson D., Aufmuth P., Aulbert C., Aylott B. E., Babak S., Baker P., Ballardin G., Ballmer S., Barayoga J. C. B., Barker D., Barone F., Barr B., Barsotti L., Barsuglia M., Barton M. A., Bartos I., Bassiri R., Bastarrika M., Basti A., Batch J., Bauchrowitz J., Bauer Th. S., Bebronne M., Beck D., Behnke B., Bejger M., Beker M. G., Bell A. S., Belletoile A., Belopolski I., Benacquista M., Berliner J. M., Bertolini A., Betzwieser J., Beveridge N., Beyersdorf P. T., Bilenko I. A., Billingsley G., Birch J., Biswas R., Bitossi M., Bizouard M. A., Black E. , Blackburn J. K., Blackburn L., Blair D., Bland B., Blom M., Bock O., Bodiya T. P., Bogan C., Bondarescu R., Bondu F., Bonelli L., Bonnand R., Bork R., Born M., Boschi V., Bose S., Bosi L., Bouhou B., Braccini S., Bradaschia C., Brady P. R., Braginsky V. B., Branchesi M., Brau J. E., Breyer J., Briant T., Bridges D. O., Brillet A., Brinkmann M., Brisson V., Britzger M., Brooks A. F., Brown D. A., Bulik T., Bulten H. J., Buonanno A., Burguet–Castell J., Buskulic D., Buy C., Byer R. L., Cadonati L., Cagnoli G., Calloni E., Camp J. B., Campsie P., Cannizzo J., Cannon K., Canuel B., Cao J., Capano C. D., Carbognani F., Carbone L., Caride S., Caudill S., Cavaglià M., Cavalier F., Cavalieri R., Cella G., Cepeda C., Cesarini E., Chaibi O., Chalermsongsak T., Charlton P., Chassande-Mottin E., Chelkowski S., Chen W., Chen X., Chen Y., Chincarini A., Chiummo A., Cho H. S., Chow J., Christensen N., Chua S. S. Y., Chung C. T. Y., Chung S., Ciani G., Clara F., Clark D. E., Clark J., Clayton J. H., Cleva F., Coccia E., Cohadon P.-F., Colacino C. N., Colas J., Colla A., Colombini M., Conte A., Conte R., Cook D., Corbitt T. R., Cordier M., Cornish N., Corsi A., Costa C. A., Coughlin M., Coulon J.-P., Couvares P., Coward D. M., Cowart M., Coyne D. C., Creighton J. D. E., Creighton T. D., Cruise A. M., Cumming A., Cunningham L., Cuoco E., Cutler R. M., Dahl K., Danilishin S. L., Dannenberg R., D’Antonio S., Danzmann K., Dattilo V., Daudert B., Daveloza H., Davier M., Daw E. J., Day R., Dayanga T., De Rosa R., DeBra D., Debreczeni G., Del Pozzo W., del Prete M., Dent T., Dergachev V., DeRosa R., DeSalvo R., Dhurandhar S., Di Fiore L., Di Lieto A., Di Palma I., Di Paolo Emilio M., Di Virgilio A., Díaz M., Dietz A., Donovan F., Dooley K. L., Drago M., Drever R. W. P., Driggers J. C., Du Z., Dumas J.-C., Dwyer S., Eberle T., Edgar M., Edwards M., Effler A., Ehrens, P., Endrőczi G., Engel R., Etzel T., Evans K., Evans M., Evans T., Factourovich M., Fafone V., Fairhurst S., Fan Y., Farr B. F., Fazi D., Fehrmann H., Feldbaum D., Feroz F., Ferrante I., Fidecaro F., Finn L. S., Fiori I., Fisher R. P., Flaminio R., Flanigan M., Foley S., Forsi E., Forte L. A., 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., Fujimoto M.-K., Fulda P. J., Fyffe M., Gair J., Galimberti M., Gammaitoni L., Garcia J., Garufi F., Gáspár M. E., Gemme G., Geng R., Genin E., Gennai A., Gergely L. Á., Ghosh S., Giaime J. A., Giampanis S., Giardina K. D., Giazotto A., Gil-Casanova S., Gill C., Gleason J., Goetz E., Goggin L. M., González G., Gorodetsky M. L., Goßler S., Gouaty R., Graef C., Graff P. B., Granata M., Grant A., Gras S., Gray C., Gray N., Greenhalgh R. J. S., Gretarsson A. M., Greverie C., Grosso R., Grote H., Grunewald S., Guidi G. M., Guido C., Gupta R., Gustafson E. K., Gustafson R., Ha T., Hallam J. M., Hammer D., Hammond G., Hanks J., Hanna C., Hanson J., Harms J., Hardt A., Harry G. M., Harry I. W., Harstad E. D., Hartman M. T., Haughian K., Hayama K., Hayau J.-F., Heefner J., Heidmann A., Heintze M. C., Heitmann H., Hello P., Hendry M. A., Heng I. S., Heptonstall A. W., Herrera V., Hewitson M., Hild S., Hoak D., Hodge K. A., Holt K., Holtrop M., Hong T., Hooper S., Hosken D. J., Hough J., Howell E. J., Hughey B., Husa S., Huttner S. H., Huynh-Dinh T., Ingram D. R., Inta R., Isogai T., Ivanov A., Izumi K., Jacobson M., James E., Jang Y. J., Jaranowski P., Jesse E., Johnson W. W., Jones D. I., Jones G., Jones R., Ju L., Kalmus P., Kalogera V., Kandhasamy S., Kang G., Kanner J. B., Kasturi R., Katsavounidis E., Katzman W., Kaufer H., Kawabe K., Kawamura S., Kawazoe F., Kelley D., Kells W., Keppel D. G., Keresztes Z., Khalaidovski A., Khalili F. Y., Khazanov E. A., Kim B. K., Kim C., Kim H., Kim K., Kim N., Kim Y. M., King P. J., Kinze D. L., Kissel J. S., Klimenko S., Kokeyama K., Kondrashov V., Koranda S., Korth W. Z., Kowalska I., Kozak D., Kranz O., Kringel V., Krishnamurthy S., Krishnan B., Królak A., Kuehn G., Kumar R.,. Kwee P., Lam P. K., Landry M., Lantz B., Lastzka N., Lawrie C., Lazzarini A., Leaci P., Lee C. H., Lee H. K., Lee H. M., Leong J. R., Leonor I., Leroy N., Letendre N., Li J., Li T. G. F., Liguori N., Lindquist P. E., Liu Y., Liu Z., Lockerbie N. A., Lodhia D., Lorenzini M., Loriette V., Lormand M., Losurdo G., Lough J., Luan J., Lubinski M., Lück H., Lundgren A. P., Macdonald E., Machenschalk B., MacInnis M., Macleod D. M., Mageswaran M., Mailand K., Majorana E., Maksimovic I., Man N., Mandel I., Mandic V., Mantovani M., Marandi A., Marchesoni F., Marion F., Márka S., Márka Z., Markosyan A., 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., Mazzolo G., McCarthy R., McClelland D. E., McGuire S. C., McIntyre G., McIver J., McKechan D. J. A., McWilliams S., Meadors G. D., Mehmet M., Meier T., Melatos A., Melissinos A. C., Mendell G., Mercer R. A., Meshkov S., Messenger C., Meyer M. S., Miao H., Michel C., Milano L., Miller J., Minenkov Y., Mitrofanov V. P., Mitselmakher G., Mittleman R., Miyakawa O., Moe B., Mohan M., Mohanty S. D., Mohapatra S. R. P., Moraru D., Moreno G., Morgado N., Morgia A., Mori T., Morriss S. R., Mosca S., Mossavi K., Mours B., Mow–Lowry C. M., Mueller C. L., Mueller G., Mukherjee S., Mullavey A., Müller-Ebhardt H., Munch J., Murphy D., Murray P. G., Mytidis A., Nash T., Naticchioni L., Necula V., Nelson J., Neri I., Newton G., Nguyen T., Nishizawa A., Nitz A., Nocera F., Nolting D., Normandin M. E., Nuttall L., Ochsner E., O’Dell J., Oelker E., Ogin G. H., Oh J. J., Oh S. H., O’Reilly B., O’Shaughnessy R., Osthelder C., Ott C. D., Ottaway D. J., Ottens R. S., Overmier H., Owen B. J., Page A., Pagliaroli G., Palladino L., Palomba C., Pan Y., Pankow C., Paoletti F., Papa M. A., Parisi M., Pasqualetti A., Passaquieti R., Passuello D., Patel P., Pedraza M., Peiris P., Pekowsky L., Penn S., Perreca A., Persichetti G., Phelps M., Pichot M., Pickenpack M., Piergiovanni F., Pietk M., Pinard L., Pinto I. M., Pitkin M., Pletsch H. J., Plissi M. V., Poggiani R., Pöld J., Postiglione F., Prato M., Predoi V., Prestegard T., Price L. R., Prijatelj M., Principe M., Privitera S., Prix R., Prodi G. A., Prokhorov L. G., Puncken O., Punturo M., Puppo P., Quetschke V., Quitzow-James R., Raab F. J., Rabeling D. S., Rácz I., Radkins H., Raffai P., Rakhmanov M., Rankins B., Rapagnani P., Raymond V., Re V., Redwine K., Reed C. M., Reed T., Regimbau T., Reid S., Reitze D. H., Ricci F., Riesen R., Riles K., Robertson N. A., Robinet F., Robinson C., Robinson E. L., Rocchi A., Roddy S., Rodriguez C., Rodruck M., Rolland L., Rollins J. G., Romano J. D., Romano R., Romie J. H., Rosińska D., Röver C., Rowan S., Rüdiger A., Ruggi P., Ryan K., Sainathan P., Salemi F., Sammut L., Sandberg V., Sannibale V., Santamaría L., Santiago-Prieto I., Santostasi G., Sassolas B., Sathyaprakash B. S., Sato S., Saulson P. R., Savage R. L., Schilling R., Schnabel R., Schofield R. M. S., Schreiber E., Schulz B., Schutz B. F., Schwinberg P., Scott J., Scott S. M., Seifert F., Sellers D., Sentenac D., Sergeev A., Shaddock D. A., Shaltev M., Shapiro B., Shawhan P., Shoemaker D. H., Sibley A., Siemens X., Sigg D., Singer A., Singer L., Sintes A. M., Skelton G. R., Slagmolen B. J. J., Slutsky J., Smith J. R., Smith M. R., Smith R. J. E., Smith-Lefebvre N. D., Somiya K., Sorazu B., Soto J., Speirits F. C., Sperandio L., Stefszky M., Stein A. J., Stein L. C., Steinert E., Steinlechner J., Steinlechner S., Steplewski S., Stochino A., Stone R., Strain K. A., Strigin S. E., Stroeer A. S., Sturani R., Stuver A. L., Summerscales T. Z., Sung M., Susmithan S., Sutton P. J., Swinkels B., Tacca M., Taffarello L., Talukder D., Tanner D. B., Tarabrin S. P., Taylor J. R., Taylor R., Thomas P., Thorne K. A., Thorne K. S., Thrane E., Thüring A., Tokmakov K. V., Tomlinson C., Toncelli A., Tonelli M., Torre O., Torres C., Torrie C. I., Tournefier E., Travasso F., Traylor G., Tseng K., Tucker E., Ugolini D., Vahlbruch H., Vajente G., van den Brand J. F. J., Van Den Broeck C., van der Putten S., van Veggel A. A., Vass S., Vasuth M., Vaulin R., Vavoulidis M., Vecchio A., Vedovato G., Veitch J., Veitch P. J., Veltkamp C., Verkindt D., Vetrano F., Viceré A., Villar A. E., Vinet J.-Y., Vitale S., Vocca H., Vorvick C., Vyatchanin S. P., Wade A., Wade L., Wade M., Waldman S. J., Wallace L., Wan Y., Wang M., Wang X., Wang Z., Wanner A., Ward R. L., Was M., Weinert M., Weinstein A. J., Weiss R., Wen L., Wessels P., West M., Westphal T., Wette K., Whelan J. T., Whitcomb S. E., White D. J., Whiting B. F., Wilkinson C., Willems P. A., Williams L., Williams R., Willke B., Winkelmann L., Winkler W., Wipf C. C., Wiseman A. G., Wittel H., Woan G., Wooley R., Worden J., Yakushin I., Yamamoto H., Yamamoto K., Yancey C. C., Yang H., Yeaton-Massey D., Yoshida S., Yu P., Yvert M., Zadrożny A., Zanolin M., Zendri J.-P., Zhang F., Zhang L., Zhang W., Zhao C., Zotov N., Zucker M. E., Zweizig J.

Autors Affiliation: LIGO – California Institute of Technology, Pasadena, California 91125, USA
2California State University Fullerton, Fullerton California 92831 USA
3SUPA, University of Glasgow, Glasgow, G12 8QQ, United Kingdom
4Laboratoire d’Annecy-le-Vieux de Physique des Particules (LAPP), Université de Savoie, CNRS/IN2P3, F-74941 Annecy-Le-Vieux, France
5aINFN, Sezione di Napoli, I-84084 Salerno, Italy
5bUniversità di Napoli ’Federico II’, Complesso Universitario di Monte S. Angelo, I-80126 Napoli, I-84084 Salerno, Italy
5cUniversità di Salerno, Fisciano, I-84084 Salerno, Italy
6LIGO – Livingston Observatory, Livingston, Louisiana 70754, USA
7Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
8Leibniz Universität Hannover, D-30167 Hannover, Germany
9aNikhef, Science Park, Amsterdam, the Netherlands, 1081 HV Amsterdam, the Netherlands
9bVU University Amsterdam, De Boelelaan 1081, 1081 HV Amsterdam, the Netherlands
10National Astronomical Observatory of Japan, Tokyo 181-8588, Japan
11University of Wisconsin–Milwaukee, Milwaukee, Wisconsin 53201, USA
12University of Florida, Gainesville, Florida 32611, USA
13University of Birmingham, Birmingham, B15 2TT, United Kingdom
14aINFN, Sezione di Roma, I-00185 Roma, Italy
14bUniversità ’La Sapienza’, I-00185 Roma, Italy
15LIGO – Hanford Observatory, Richland, Washington 99352, USA
16Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-14476 Golm, Germany
17Montana State University, Bozeman, Montana 59717, USA
18European Gravitational Observatory (EGO), I-56021 Cascina (PI), Italy
19Syracuse University, Syracuse, New York 13244, USA
20LIGO – Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
21APC, AstroParticule et Cosmologie, Université Paris Diderot, CNRS/IN2P3, CEA/Irfu, Observatoire de Paris, Sorbonne Paris Cité, 10, rue Alice Domon et Léonie Duquet, 75205 Paris Cedex 13, France
22Columbia University, New York, New York 10027, USA
23aINFN, Sezione di Pisa, I-53100 Siena, Italy
23bUniversità di Pisa; I-56127 Pisa, I-53100 Siena, Italy
23cUniversità di Siena, I-53100 Siena, Italy
24Stanford University, Stanford, California 94305, USA
25aIM-PAN 00-956 Warsaw, Poland
25bAstronomical Observatory Warsaw University, 00-478 Warsaw, Poland
25cCAMK-PAN, 00-716 Warsaw, Poland
25dBiałystok University, 15-424 Białystok, Poland
25eNCBJ, 05-400 Świerk-Otwock, Poland
25fInstitute of Astronomy, 65-265 Zielona Góra, Poland
26The University of Texas at Brownsville and Texas Southmost College, Brownsville, Texas 78520, USA
27San Jose State University, San Jose, California 95192, USA
28Moscow State University, Moscow, 119992, Russia
29aLAL, Université Paris-Sud, IN2P3/CNRS, F-91898 Orsay, France
29bESPCI, CNRS, F-75005 Paris, France
30NASA/Goddard Space Flight Center, Greenbelt, Maryland 20771, USA
31University of Western Australia, Crawley, WA 6009, Australia
32The Pennsylvania State University, University Park, Pennsylvania 16802, USA
33aUniversité Nice-Sophia-Antipolis, CNRS, Observatoire de la Côte d’Azur, F-06304 Nice, France
33bInstitut de Physique de Rennes, CNRS, Université de Rennes 1, 35042 Rennes, France
34Laboratoire des Matériaux Avancés (LMA), IN2P3/CNRS, F-69622 Villeurbanne, Lyon, France
35Washington State University, Pullman, Washington 99164, USA
36aINFN, Sezione di Perugia, I-06123 Perugia, Italy
36bUniversità di Perugia, I-06123 Perugia, Italy
37aINFN, Sezione di Firenze, I-50019 Sesto Fiorentino, Italy
37bUniversità degli Studi di Urbino ’Carlo Bo’, I-61029 Urbino, Italy
38University of Oregon, Eugene, Oregon 97403, USA
39Laboratoire Kastler Brossel, ENS, CNRS, UPMC, Université Pierre et Marie Curie, 4 Place Jussieu, F-75005 Paris, France
40University of Maryland, College Park, Maryland 20742 USA
41Universitat de les Illes Balears, E-07122 Palma de Mallorca, Spain
42University of Massachusetts – Amherst, Amherst, Massachusetts 01003, USA
43Canadian Institute for Theoretical Astrophysics, University of Toronto, Toronto, Ontario, M5S 3H8, Canada
44Tsinghua University, Beijing 100084 China
45University of Michigan, Ann Arbor, Michigan 48109, USA
46Louisiana State University, Baton Rouge, Louisiana 70803, USA
47The University of Mississippi, University, Mississippi 38677, USA
48Charles Sturt University, Wagga Wagga, NSW 2678, Australia
49Caltech-CaRT, Pasadena, California 91125, USA
50INFN, Sezione di Genova, I-16146 Genova, Italy
51Pusan National University, Busan 609-735, Korea
52Australian National University, Canberra, ACT 0200, Australia
53Carleton College, Northfield, Minnesota 55057, USA
54The University of Melbourne, Parkville, VIC 3010, Australia
55Cardiff University, Cardiff, CF24 3AA, United Kingdom
56aINFN, Sezione di Roma Tor Vergata, Italy
56bUniversità di Roma Tor Vergata, I-00133 Roma, Italy
56cUniversità dell’Aquila, I-67100 L’Aquila, Italy
57University of Salerno, I-84084 Fisciano (Salerno), Italy and INFN (Sezione di Napoli), Italy
58The University of Sheffield, Sheffield S10 2TN, United Kingdom
59WIGNER RCP, RMKI, H-1121 Budapest, Konkoly Thege Miklós út 29-33, Hungary
60aINFN, Gruppo Collegato di Trento, I-38050 Povo, Trento, Italy
60bUniversità di Trento, I-38050 Povo, Trento, Italy
60cINFN, Sezione di Padova, I-35131 Padova, Italy
60dUniversità di Padova, I-35131 Padova, Italy
61Inter-University Centre for Astronomy and Astrophysics, Pune – 411007, India
62California Institute of Technology, Pasadena, California 91125, USA
63Northwestern University, Evanston, Illinois 60208, USA
64University of Cambridge, Cambridge, CB2 1TN, United Kingdom
65The University of Texas at Austin, Austin, Texas 78712, USA
66Rochester Institute of Technology, Rochester, New York 14623, USA
67Eötvös Loránd University, Budapest, 1117 Hungary
68University of Szeged, 6720 Szeged, Dóm tér 9, Hungary
69Rutherford Appleton Laboratory, HSIC, Chilton, Didcot, Oxon OX11 0QX United Kingdom
70Embry-Riddle Aeronautical University, Prescott, Arizona 86301 USA
71National Institute for Mathematical Sciences, Daejeon 305-390, Korea
72Perimeter Institute for Theoretical Physics, Ontario, N2L 2Y5, Canada
73University of New Hampshire, Durham, New Hampshire 03824, USA
74University of Adelaide, Adelaide, SA 5005, Australia
75University of Southampton, Southampton, SO17 1BJ, United Kingdom
76University of Minnesota, Minneapolis, Minnesota 55455, USA
77Korea Institute of Science and Technology Information, Daejeon 305-806, Korea
78Hobart and William Smith Colleges, Geneva, New York 14456, USA
79Institute of Applied Physics, Nizhny Novgorod, 603950, Russia
80Lund Observatory, Box 43, SE-221 00, Lund, Sweden
81Hanyang University, Seoul 133-791, Korea
82Seoul National University, Seoul 151-742, Korea
83University of Strathclyde, Glasgow, G1 1XQ, United Kingdom
84Southern University and A&M College, Baton Rouge, Louisiana 70813, USA
85University of Rochester, Rochester, New York 14627, USA
86University of Sannio at Benevento, I-82100 Benevento, Italy and INFN (Sezione di Napoli), Italy
87Louisiana Tech University, Ruston, Louisiana 71272, USA
88McNeese State University, Lake Charles, Louisiana 70609 USA
89Andrews University, Berrien Springs, Michigan 49104 USA
90Trinity University, San Antonio, Texas 78212, USA
91Southeastern Louisiana University, Hammond, Louisiana 70402, USA

Abstract: We present results from a search for gravitational-wave bursts in the data collected by the LIGO and Virgo detectors between July 7, 2009 and October 20, 2010: data are analyzed when at least two of the three LIGO-Virgo detectors are in coincident operation, with a total observation time of 207 days. The analysis searches for transients of duration less than or similar to 1 s over the frequency band 64-5000 Hz, without other assumptions on the signal waveform, polarization, direction or occurrence time. All identified events are consistent with the expected accidental background. We set frequentist upper limits on the rate of gravitational-wave bursts by combining this search with the previous LIGO-Virgo search on the data collected between November 2005 and October 2007. The upper limit on the rate of strong gravitational-wave bursts at the Earth is 1.3 events per year at 90% confidence. We also present upper limits on source rate density per year and Mpc(3) for sample populations of standard-candle sources. As in the previous joint run, typical sensitivities of the search in terms of the root-sum-squared strain amplitude for these waveforms lie in the range similar to 5 x 10(-22) Hz(-1/2) to similar to 1 x 10(-20) Hz(-1/2). The combination of the two joint runs entails the most sensitive all-sky search for generic gravitational-wave bursts and synthesizes the results achieved by the initial generation of interferometric detectors.

Journal/Review: PHYSICAL REVIEW D

Volume: 85 (12)      Pages from: 122007  to: 122007

More Information: 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 GEO 600 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 the support of the research 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 Polish Ministry of Science and Higher Education, the FOCUS Programme of Foundation for Polish Science, 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. This document has been assigned LIGO Laboratory document number LIGO-P1100118-v16.
KeyWords: gravitational waves; LIGO; Virgo; science run; detectors
DOI: 10.1103/PhysRevD.85.122007

Citations: 97
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