Abbott, B. P. and Abbott, R. and Adhikari, Rana X. and Ageev, A. and Allen, B. and Amin, R. and Anderson, S. B. and Anderson, W. G. and Araya, M. and Armandula, H. and Ashley, M. and Asiri, F. and Aufmuth, P. and Aulbert, C. and Babak, S. and Balasubramanian, R. and Ballmer, S. and Barish, B. C. and Barker, C. and Barker, D. and Barnes, M. and Barr, B. and Barton, M. A. and Bayer, K. and Beausoleil, R. and Belczynski, K. and Bennett, R. and Berukoff, S. J. and Betzwieser, J. and Bhawal, B. and Bilenko, I. A. and Billingsley, G. and Black, E. and Blackburn, K. and Blackburn, L. and Bland, B. and Bochner, B. and Bogue, L. and Bork, R. and Bose, S. and Brady, P. R. and Braginsky, V. B. and Brau, J. E. and Brown, D. A. and Bullington, A. and Bunkowski, A. and Buonanno, A. and Burgess, R. and Busby, D. and Butler, W. E. and Byer, R. L. and Cadonati, L. and Cagnoli, G. and Camp, J. B. and Cantley, C. A. and Cardenas, L. and Carter, K. and Casey, M. M. and Castiglione, J. and Chandler, A. and Chapsky, J. and Charlton, P. and Chatterji, S. and Chelkowski, S. and Chen, Y. and Chickarmane, V. and Chin, D. and Christensen, N. and Churches, D. and Cokelaer, T. and Colacino, C. and Coldwell, R. and Coles, M. and Cook, D. and Corbitt, T. and Coyne, D. and Creighton, J. D. E. and Creighton, T. D. and Crooks, D. R. M. and Csatorday, P. and Cusack, B. J. and Cutler, C. and D’Ambrosio, E. and Danzmann, K. and Daw, E. and DeBra, D. and Delker, T. and Dergachev, V. and DeSalvo, R. and Dhurandhar, S. and Di Credico, A. and Díaz, M. and Ding, H. and Drever, R. W. P. and Dupuis, R. J. and Edlund, J. A. and Ehrens, P. and Elliffe, E. J. and Etzel, T. and Evans, M. and Evans, T. and Fairhurst, S. and Fallnich, C. and Farnham, D. and Fejer, M. M. and Findley, T. and Fine, M. and Finn, L. S. and Franzen, K. Y. and Freise, A. and Frey, R. and Fritschel, P. and Frolov, V. V. and Fyffe, M. and Ganezer, K. S. and Garofoli, J. and Giaime, J. A. and Gillespie, A. and Goda, K. and González, G. and Goßler, S. and Grandclément, P. and Grant, A. and Gray, C. and Gretarsson, A. M. and Grimmett, D. and Grote, H. and Grunewald, S. and Guenther, M. and Gustafson, E. and Gustafson, R. and Hamilton, W. O. and Hammond, M. and Hanson, J. and Hardham, C. and Harms, J. and Harry, G. and Hartunian, A. and Heefner, J. and Hefetz, Y. and Heinzel, G. and Heng, I. S. and Hennessy, M. and Hepler, N. and Heptonstall, A. and Heurs, M. and Hewitson, M. and Hild, S. and Hindman, N. and Hoang, P. and Hough, J. and Hrynevych, M. and Hua, W. and Ito, M. and Itoh, Y. and Ivanov, A. and Jennrich, O. and Johnson, B. and Johnson, W. W. and Johnston, W. R. and Jones, D. I. and Jones, L. and Jungwirth, D. and Kalogera, V. and Katsavounidis, E. and Kawabe, K. and Kawamura, S. and Kells, W. and Kern, J. and Khan, A. and Killbourn, S. and Killow, C. J. and Kim, C. and King, C. and King, P. and Klimenko, S. and Koranda, S. and Kötter, K. and Kovalik, J. and Kozak, D. and Krishnan, B. and Landry, M. and Langdale, J. and Lantz, B. and Lawrence, R. and Lazzarini, A. and Lei, M. and Leonor, I. and Libbrecht, K. and Libson, A. and Lindquist, P. and Liu, S. and Logan, J. and Lormand, M. and Lubinski, M. and Lück, H. and Lyons, T. T. and Machenschalk, B. and MacInnis, M. and Mageswaran, M. and Mailand, K. and Majid, W. and Malec, M. and Mann, F. and Marin, A. and Márka, S. and Maros, E. and Mason, J. and Mason, K. and Matherny, O. and Matone, L. and Mavalvala, N. and McCarthy, R. and McClelland, D. E. and McHugh, M. and McNabb, J. W. C. and Mendell, G. and Mercer, R. A. and Meshkov, S. and Messaritaki, E. and Messenger, C. and Mitrofanov, V. P. and Mitselmakher, G. and Mittleman, R. and Miyakawa, O. and Miyoki, S. and Mohanty, S. and Moreno, G. and Mossavi, K. and Mueller, G. and Mukherjee, S. and Murray, P. and Myers, J. and Nagano, S. and Nash, T. and Nayak, R. and Newton, G. and Nocera, F. and Noel, J. S. and Nutzman, P. and Olson, T. and O'Reilly, B. and Ottaway, D. J. and Ottewill, A. and Ouimette, D. and Overmier, H. and Owen, J. and Pan, Y. and Papa, M. A. and Parameshwaraiah, V. and Parameswaran, A. and Parameswariah, C. and Pedraza, M. and Penn, S. and Pitkin, M. and Plissi, M. and Prix, R. and Quetschke, V. and Raab, F. and Radkins, H. and Rahkola, R. and Rakhmanov, M. and Rao, S. R. and Rawlins, K. and Ray-Majumder, S. and Re, V. and Redding, D. and Regehr, M. W. and Regimbau, T. and Reid, S. and Reilly, K. T. and Reithmaier, K. and Reitze, D. H. and Richman, S. and Riesen, R. and Riles, K. and Rivera, B. and Rizzi, A. and Robertson, D. I. and Robertson, N. A. and Robison, L. and Roddy, S. and Rollins, J. and Romano, J. D. and Romie, J. and Rong, H. and Rose, D. and Rotthoff, E. and Rowan, S. and Rüdiger, A. and Russell, P. and Ryan, K. and Salzman, I. and Sandberg, V. and Sanders, G. H. and Sannibale, V. and Sathyaprakash, B. and Saulson, P. R. and Savage, R. and Sazonov, A. and Schilling, R. and Schlaufman, K. and Schmidt, V. and Schnabel, R. and Schofield, R. and Schutz, B. F. and Schwinberg, P. and Scott, S. M. and Seader, S. E. and Searle, A. C. and Sears, B. and Seel, S. and Seifert, F. and Sengupta, A. S. and Shapiro, C. A. and Shawhan, P. and Shoemaker, D. H. and Shu, Q. Z. and Sibley, A. and Siemens, X. and Sievers, L. and Sigg, D. and Sintes, A. M. and Smith, R. and Smith, M. and Smith, M. R. and Sneddon, P. H. and Spero, R. and Stapfer, G. and Steussy, D. and Strain, K. A. and Strom, D. and Stuver, A. and Summerscales, T. and Sumner, M. C. and Sutton, P. J. and Sylvestre, J. and Takamori, A. and Tanner, D. B. and Tariq, H. and Taylor, I. and Taylor, R. and Taylor, R. and Thorne, K. A. and Thorne, K. S. and Tibbits, M. and Tilav, S. and Tinto, M. and Tokmakov, K. V. and Torres, C. and Torrie, C. and Traylor, G. and Tyler, W. and Ugolini, D. and Ungarelli, C. and Vallisneri, M. and van Putten, M. and Vass, S. and Vecchio, A. and Veitch, J. and Vorvick, C. and Vyachanin, S. P. and Wallace, L. and Walther, H. and Ward, H. and Ware, B. and Watts, K. and Webber, D. and Weidner, A. and Weiland, U. and Weiss, R. and Welling, H. and Wen, L. and Wen, S. and Whelan, J. T. and Whitcomb, S. E. and Whiting, B. F. and Wiley, S. and Wilkinson, C. and Willems, P. A. and Williams, P. R. and Williams, R. and Willke, B. and Wilson, A. and Winjum, B. J. and Winkler, W. and Wise, S. and Wiseman, A. G. and Woan, G. and Woods, D. and Wooley, R. and Worden, J. and Wu, W. and Yakushin, I. and Yamamoto, H. and Yoshida, S. and Zaleski, K. D. and Zanolin, M. and Zawischa, I. and Zhang, L. and Zhu, R. and Zotov, N. and Zucker, M. and Zweizig, J. and Weinstein, Alan J. (2005) Search for gravitational waves from galactic and extra-galactic binary neutron stars. Physical Review D, 72 (8). Art. No. 082001. ISSN 0556-2821. http://resolver.caltech.edu/CaltechAUTHORS:ABBprd05d
- Published Version
See Usage Policy.
Use this Persistent URL to link to this item: http://resolver.caltech.edu/CaltechAUTHORS:ABBprd05d
We use 373 hours (≈15 days) of data from the second science run of the LIGO gravitational-wave detectors to search for signals from binary neutron star coalescences within a maximum distance of about 1.5 Mpc, a volume of space which includes the Andromeda Galaxy and other galaxies of the Local Group of galaxies. This analysis requires a signal to be found in data from detectors at the two LIGO sites, according to a set of coincidence criteria. The background (accidental coincidence rate) is determined from the data and is used to judge the significance of event candidates. No inspiral gravitational-wave events were identified in our search. Using a population model which includes the Local Group, we establish an upper limit of less than 47 inspiral events per year per Milky Way equivalent galaxy with 90% confidence for nonspinning binary neutron star systems with component masses between 1 and 3M☉.
|Additional Information:||© 2005 American Physical Society. Received 30 May 2005; published 25 October 2005. The authors gratefully acknowledge the support of the United States National Science Foundation for the construction and operation of the LIGO Laboratory, and the Particle Physics and Astronomy Research 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. The authors also gratefully acknowledge the support of the research by these agencies and by the Australian Research Council, the Natural Sciences and Engineering Research Council of Canada, the Council of Scientific and Industrial Research of India, the Department of Science and Technology of India, the Spanish Ministerio de Educacion y Ciencia, the John Simon Guggenheim Foundation, the Leverhulme Trust, the David and Lucile Packard Foundation, the Research Corporation, and the Alfred P. Sloan Foundation.|
|Usage Policy:||No commercial reproduction, distribution, display or performance rights in this work are provided.|
|Deposited By:||Tony Diaz|
|Deposited On:||02 Feb 2009 20:42|
|Last Modified:||11 Sep 2014 17:40|
Repository Staff Only: item control page