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          Document History for Document ID 368250

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Document Version Version Comment Date Status
368250.0 [No comment] 06.04.2009 15:01 Released

ID: 368250.0, MPI für Gravitationsphysik / Laser Interferometry & Gravitational Wave Astronomy
Analysis of LIGO data for gravitational waves from binary neutron stars
Authors:Abbott, B.; Abbott, F.; Adhikari, R.; Ageev, A.; Allen, Bruce; Amin, R.; Anderson, S. B.; Anderson, W. G.; Araya, M.; Armandula, H.; Asiri, F.; Aufmuth, Peter; Aulbert, Carsten; Babak, Stanislav; Balasubramanian, R.; Ballmer, S.; Barish, B. C.; Barker, D.; Barker-Patton, C.; Barnes, M.; Barr, B. W.; Barton, M. A.; Bayer, K.; Beausoleil, R.; Belczynski, K.; Bennett, R.; Berukoff, Steven J.; Betzwieser, J.; Bhawal, B.; Bilenko, I. A.; Billingsley, G.; Black, E.; Blackburn, K.; Bland-Weaver, B.; Bochner, B.; Bogue, L.; Bork, Rolf; Bose, Sukanta; Brady, Patrick R.; Braginsky, V. B.; Brau, J. E.; Brown, Duncan A.; Brozek, Oliver Sascha; Bullington, A.; Buonanno, Alessandra; Burgess, R.; Busby, D.; Butler, W. E.; Byer, R. L.; Cadonati, L.; Cagnoli, G.; Camp, J. B.; Cantley, C. A.; Cardenas, L.; Carter, K.; Casey, Morag M.; Castiglione, J.; Chandler, A.; Chapsky, J.; Charlton, P.; Chatterji, S.; Chen, Yanbei; Chickarmane, V.; Chin, D.; Christensen, Nelson; Churches, D.; Colacino, Carlo Nicola; Coldwell, R.; Coles, M.; Cook, D.; Corbitt, Thomas; Coyne, D.; Creighton, Jolien D. E.; Creighton, Teviet D.; Crooks, D. R. M.; Csatorday, P.; Cusack, B. J.; Cutler, Curt; D'Ambrosio, Erika; Danzmann, Karsten; Davies, R.; Daw, Edward J.; DeBra, D.; Delker, T.; DeSalvo, R.; Dhurandhar, Sanjeev; Diaz, M.; Ding, H.; Drever, R. W. P.; Dupuis, R. J.; Ebeling, C.; Edlund, J. A.; Ehrens, P.; Elliffe, E. J.; Etzel, T.; Evans, M.; Evans, T.; Fallnich, Carsten; Farnham, D.; Fejer, M. M.; Fine, M.; Finn, Lee S.; Flanagan, Eanna E.; Freise, Andreas; Frey, R.; Fritschel, P.; Frolov, V. V.; Ganezer, K. S.; Giaime, J. A.; Gillespie, A.; Goda, Keisuke; Gonzalez, Gabriela; Gossler, Stefan; Grandclement, P.; Grant, A.; Gray, C.; Gretarsson, A. M.; Grimmett, D.; Grote, Hartmut; Grunewald, Steffen; Guenther, Mathias; Gustafson, E. K.; Gustafson, R.; Hamilton, W. O.; Hammond, M.; Hanson, J.; Hardham, C.; Harry, G.; Hartunian, A.; Heefner, J.; Hefetz, Y.; Heinzel, Gerhard; Heng, Ik Siong; Hennessy, M.; Hepler, N.; Heptonstall, A.; Heurs, Michele; Hewitson, Martin; Hindman, N.; Hoang, P.; Hough, Jim; Hrynevych, M.; Hua, W.; Ingley, R.; Ito, M.; Itoh, Yousuke; Ivanov, A.; Jennrich, Oliver; Johnson, W. W.; Johnston, W. R.; Jones, L.; Jungwirth, D.; Kalogera, V.; Katsavounidis, E.; Kawabe, Keita; Kawamura, Seiji; Kells, W.; Kern, J.; Khan, A.; Killbourn, S.; Killow, Christian J.; Kim, C.; King, C.; King, Peter; Klimenko, S.; Kloevekorn, P.; Koranda, S.; Kötter, Karsten; Kovalik, J.; Kozak, D.; Krishnan, Badri; Landry, Michael; Langdale, J.; Lantz, B.; Lawrence, R.; Lazzarini, Albert; Lei, M.; Leonhardt, Volker; Leonor, I.; Libbrecht, K.; Lindquist, P.; Liu, S.; Logan, J. E.; Lormand, M.; Lubinski, M.; Lück, Harald; Lyons, T. T.; Machenschalk, Bernd; MacInnis, M.; Mageswaran, M.; Mailand, K.; Majid, W.; Malec, Michaela; Mann, F.; Marin, A.; Marka, S.; Maros, E.; Mason, J.; Matherny, O.; Mason, K.; Matone, L.; Mavalvala, N.; McCarthy, R.; McClelland, D. E.; McHugh, Martin; McNamara, P. W.; Mendell, Gregory; Meshkov, S.; Messenger, Christopher; Mitrofanov, V. P.; Mitselmakher, G.; Mittleman, R.; Miyakawa, O.; Miyoki, Shinji; Mohanty, Soumya; Moreno, G.; Mossavi, Kasem; Mours, B.; Müller, G.; Mukherjee, Soma; Myers, J.; Naganov, S.; Nash, T.; Naundorf, Holger; Nayak, R.; Newton, G.; Nocera, F.; Nutzman, P.; Olson, T.; O'Reilly, B.; Ottaway, D. J.; Ottewill, A.; Ouimette, D.; Overmier, H.; Owen, Benjamin J.; Papa, Maria Alessandra; Parameswariah, C.; Parameswariah, V.; Pedraza, M.; Penn, S.; Pitkin, Matthew; Plissi, M. V.; Pratt, M.; Quetschke, Volker; Raab, F.; Radkins, H.; Rahkola, R.; Rakhmanov, M.; Rao, S. R.; Redding, D.; Regehr, M. W.; Regimbau, T.; Reilly, K. T.; Reithmaier, K.; Reitze, D. H.; Richman, S.; Riesen, R.; Riles, K.; Rizzi, A.; Robertson, D. I.; Robertson, N. A.; Robison, L.; Roddy, S.; Rollins, J.; Romano, J. D.; Romie, J.; Rong, H.; Rose, D.; Rotthoff, E.; Rowan, S.; Rüdiger, Albrecht; Russell, P.; Ryan, K.; Salzman, I.; Sanders, G. H.; Sannibale, V.; Sathyaprakash, B.; Saulson, P. R.; Savage, R.; Sazonov, A.; Schilling, Roland; Schlaufman, K.; Schmidt, V.; Schofield, R.; Schrempel, M.; Schutz, Bernard F.; Schwinberg, P.; Scott, S. M.; Searle, A. C.; Sears, B.; Seel, S.; Sengupta, A. S.; Shapiro, C. A.; Shawhan, P.; Shoemaker, D. H.; Shu, Q. Z.; Sibley, A.; Siemens, X.; Sievers, L.; Sigg, D.; Sintes, Alicia M.; Skeldon, K. D.; Smith, J. R.; Smith, M.; Smith, M. R.; Sneddon, P.; Spero, R.; Stapfer, G.; Strain, Kenneth A.; Strom, D.; Stuver, A.; Summerscales, T.; Sumner, M. C.; Sutton, Patrick J.; Sylvestre, J.; Takamori, A.; Tanner, D. B.; Tariq, H.; Taylor, I.; Taylor, R.; Thorne, Kip S.; Tibbits, M.; Tilav, S.; Tinto, Massimo; Tokmakov, K. V.; Torres, C.; Torrie, C.; Traeger, S.; Traylor, G.; Tyler, W.; Ugolini, D.; Vallisneri, M.; van Putten, M.; Vass, S.; Vecchio, Alberto; Vorvick, C.; Vyachanin, S. P.; Wallace, L.; Walther, H.; Ward, H.; Ware, B.; Watts, K.; Webber, D.; Weidner, Andreas; Weiland, Uta; Weinstein, A.; Weiss, R.; Welling, Herbert; Wen, L.; Wen, S.; Whelan, John T.; Whitcomb, S. E.; Whiting, B. F.; Willems, P. A.; Williams, P. R.; Williams, R.; Willke, Benno; Wilson, A.; Winjum, B. J.; Winkler, Walter; Wise, S.; Wiseman, A. G.; Woan, G.; Wooley, R.; Worden, J.; Yakushin, I.; Yamamoto, H.; Yoshida, S.; Zawischa, Ivo; Zhang, L.; Zotov, N.; Zucker, M.; Zweizig, J.; Fyffe, M.
Language:English
Date of Publication (YYYY-MM-DD):2004
Title of Journal:Physical Review D
Volume:69
Issue / Number:12
Sequence Number of Article:122001
Review Status:not specified
Audience:Not Specified
Abstract / Description:We report on a search for gravitational waves from coalescing compact binary systems in the Milky Way and the Magellanic Clouds. The analysis uses data taken by two of the three LIGO interferometers during the first LIGO science run and illustrates a method of setting upper limits on inspiral event rates using interferometer data. The analysis pipeline is described with particular attention to data selection and coincidence between the two interferometers. We establish an observational upper limit of [script R]<1.7×102 per year per Milky Way Equivalent Galaxy (MWEG), with 90% confidence, on the coalescence rate of binary systems in which each component has a mass in the range 1–3 M[sun].
External Publication Status:published
Document Type:Article
Communicated by:Karsten Danzmann
Affiliations:MPI für Gravitationsphysik/Teilinstitut Hannover
MPI für Gravitationsphysik/GEO 600
MPI für Gravitationsphysik/Laser Interferometry & Gravitational Wave Astronomy
MPI für Gravitationsphysik/Astrophysical Relativity
MPI für Gravitationsphysik/Observational Relativity and Cosmology
Identifiers:DOI:10.1103/PhysRevD.69.122001
URL:http://link.aps.org/abstract/PRD/v69/e122001
ISSN:1089-4918
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