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Published May 2006 | Published
Journal Article Open

Joint LIGO and TAMA300 search for gravitational waves from inspiralling neutron star binaries

Abbott, B.
Abbott, R.
Adhikari, R. ORCID icon
Ageev, A.
Agresti, J.
Ajith, P. ORCID icon
Allen, B.
Allen, J.
Amin, R.
Anderson, S. B.
Anderson, W. G.
Araya, M.
Armandula,, H.
Ashley, M.
Asiri, F.
Aufmuth, P.
Aulbert, C.
Babak, S.
Balasubramanian, R.
Ballmer, S.
Barish, B. C.
Barker, C.
Barker, D.
Barnes, M.
Barr, B.
Barton, M. A.
Bayer, K.
Beausoleil, R.
Belczynski, K.
Bennett, R.
Berukoff, S. J.
Betzwieser, J.
Bhawal, B.
Bilenko, I. A.
Billingsley, G. ORCID icon
Black, E.
Blackburn, K.
Blackburn, L.
Bland, B.
Bochner, B.
Bogue, L.
Bork, R.
Bose, S. ORCID icon
Brady, P. R. ORCID icon
Braginsky, V. B.
Brau, J. E.
Brown, D. A. ORCID icon
Bullington, A.
Bunkowski, A.
Buonanno, A.
Burgess, R.
Busby, D.
Butler, W. E.
Byer, R. L. ORCID icon
Cadonati, L.
Cagnoli, G.
Camp, J. B.
Cannizzo, J.
Cannon, K.
Cantley, C. A.
Cao, J.
Cardenas, L.
Carter, K.
Casey, M. M.
Castiglione, J.
Chandler, A.
Chapsky, J.
Charlton, P.
Chatterji, S.
Chelkowski, S.
Chen, Y. ORCID icon
Chickarmane, V.
Chin, D.
Christensen, N.
Churches, D.
Cokelaer, T.
Colacino, C.
Coldwell, R.
Coles, M.
Cook, D.
Corbitt, T. ORCID icon
Coyne, D. ORCID icon
Creighton, J. D. E.
Creighton, T. D.
Crooks, D. R. M.
Csatorday, P.
Cusack, B. J.
Cutler, C.
Dalrymple, J.
D'Ambrosio, E.
Danzmann, K.
Davies, G.
Daw, E.
DeBra, D.
Delker, T.
Dergachev, V.
Desai, S.
DeSalvo, R.
Dhurandhar, S.
Di Credico, A.
Diaz, M.
Ding, H.
Drever, R. W. P.
Dupuis, R. J.
Edlund, J. A.
Ehrens, P.
Elliffe, E. J.
Etzel, T.
Evans, M.
Evans, T.
Fairhurst, S.
Fallnich, C.
Farnham, D.
Fejer, M. M. ORCID icon
Findley, T.
Fine, M.
Finn, L. S.
Franzen, K. Y.
Freise, A. ORCID icon
Frey, R.
Fritschel, P.
Frolov, V. V.
Fyffe, M.
Ganezer, K. S.
Garofoli, J.
Giaime, J. A.
Gillespie, A.
Goda, K.
Goggin, L.
Gonzalez, G.
Gossler, S.
Grandclement, P.
Grant, A.
Gray, C.
Gretarsson, A. M.
Grimmett, D.
Grote, H.
Grunewald, S.
Guenther, M.
Gustafson, E.
Gustafson, R.
Hamilton, W. O.
Hammond, M.
Hanna, C.
Hanson, J.
Hardham, C.
Harms, J. ORCID icon
Harry, G.
Hartunian, A.
Heefner, J.
Hefetz, Y.
Heinzel, G.
Heng, I. S.
Hennessy, M.
Hepler, N.
Heptonstall, A.
Heurs, M.
Hewitson, M.
Hild, S.
Hindman, N.
Hoang, P.
Hough, J.
Hrynevych, M.
Hua, W.
Ito, M.
Itoh, Y.
Ivanov, A.
Jennrich, O.
Johnson, B.
Johnson, W. W.
Johnston, W. R.
Jones, D. I.
Jones, G.
Jones, L.
Jungwirth, D.
Kalogera, V. ORCID icon
Katsavounidis, E.
Kawabe, K.
Kells, W.
Kern, J.
Khan, A.
Killbourn, S.
Killow, C. J.
Kim, C.
King, C.
King, P.
Klimenko, S.
Koranda, S.
Kötter, K.
Kovalik, J.
Kozak, D. ORCID icon
Krishnan, B.
Landry, M.
Langdale, J.
Lantz, B.
Lawrence, R.
Lazzarini, A.
Lei, M.
Leonor, I.
Libbrecht, K. G. ORCID icon
Libson, A.
Lindquist, P.
Liu, S.
Logan, J.
Lormand, M.
Lubinski, M.
Luck, H.
Luna, M.
Lyons, T. T.
Machenschalk, B.
MacInnis, M.
Mageswaran, M.
Mailand, K.
Majid, W.
Malec, M.
Mandic, V.
Mann, F.
Marin, A.
Marka, S.
Maros, E.
Mason, J.
Mason, K.
Matherny, O.
Matone, L.
Mavalvala, N.
McCarthy, R.
McClelland, D. E.
McHugh, M.
McNabb, J. W. C.
Melissinos, A.
Mendell, G.
Mercer, R. A.
Meshkov, S.
Messaritaki, E.
Messenger, C.
Mikhailov, E.
Mitra, S.
Mitrofanov, V. P.
Mitselmakher, G.
Mittleman, R.
Miyakawa, O.
Mohanty, S.
Moreno, G.
Mossavi, K.
Mueller, G. ORCID icon
Mukherjee, S.
Murray, P.
Myers, E.
Myers, J.
Nagano, S.
Nash, T.
Nayak, R.
Newton, G.
Nocera, F.
Noel, J. S.
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Olson, T.
O'Reilly, B.
Ottaway, D. J. ORCID icon
Ottewill, A.
Ouimette, D.
Overmier, H.
Owen, B. J.
Pan, Y.
Papa, M. A.
Parameshwaraiah, V.
Parameswariah, C.
Pedraza, M.
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Pitkin, M.
Plissi, M.
Prix, R.
Quetschke, V. ORCID icon
Raab, F.
Radkins, H.
Rahkola, R.
Rakhmanov, M.
Rao, S. R.
Rawlins, K.
Ray-Majumder, S.
Re, V.
Redding, D.
Regehr, M. W.
Regimbau, T.
Reid, S.
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Reithmaier, K.
Reitze, D. H.
Richman, S.
Riesen, R.
Riles, K.
Rivera, B.
Rizzi, A.
Robertson, D. I.
Robertson, N. A.
Robinson, C.
Robison, L.
Roddy, S.
Rodriguez, A.
Rollins, J.
Romano, J. D.
Romie, J.
Rong, H.
Rose, D.
Rotthoff, E.
Rowan, S.
Rüdiger, A.
Ruet, L.
Russell, P.
Ryan, K.
Salzman, I.
Sandberg, V.
Sanders, G. H.
Sannibale, V.
Sarin, P.
Sathyaprakash, B.
Saulson, P. R.
Savage, R.
Sazonov, A.
Schilling, R.
Schlaufman, K.
Schmidt, V.
Schnabel, R. ORCID icon
Schofield, R.
Schutz, B. F.
Schwinberg, P.
Scott, S. M.
Seader, S. E.
Searle, A. C.
Sears, B.
Seel, S.
Seifert, F.
Sellers, D.
Sengupta, A. S.
Shapiro, C. A.
Shawhan, P.
Shoemaker, D. H.
Shu, Q. Z.
Sibley, A.
Siemens, X.
Sievers, L.
Sigg, D.
Sintes, A. M.
Smith, J. R.
Smith, M. ORCID icon
Smith, M. R.
Sneddon, P. H.
Spero, R.
Spjeld, O.
Stapfer, G.
Steussy, D.
Strain, K. A.
Strom, D.
Stuver, A.
Summerscales, T.
Sumner, M. C.
Sung, M.
Sutton, P. J.
Sylvestre, J.
Tanner, D. B. ORCID icon
Tariq, H.
Tarallo, M.
Taylor, I.
Taylor, R.
Taylor, R.
Thorne, K. A.
Thorne, Kip S.
Tibbits, M.
Tilav, S.
Tinto, M. ORCID icon
Tokmakov, K. V.
Torres, C.
Torrie, C.
Traylor, G.
Tyler, W.
Ugolini, D.
Ungarelli, C.
Vallisneri, M. ORCID icon
van Putten, M.
Vass, S.
Vecchio, A. ORCID icon
Veitch, J.
Vorvick, C.
Vyachanin, S. P.
Wallace, L.
Walther, H.
Ward, H.
Ward, R.
Ware, B.
Watts, K.
Webber, D.
Weidner, A.
Weiland, U.
Weiss, R.
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Whitcomb, S. E.
Whiting, B. F. ORCID icon
Wiley, S.
Wilkinson, C.
Willems, P. A.
Williams, P. R.
Williams, R. ORCID icon
Willke, B.
Wilson, A.
Winjum, B. J.
Winkler, W.
Wise, S.
Wiseman, A. G.
Woan, G.
Woods, D.
Wooley, R.
Worden, J.
Wu, W.
Yakushin, I.
Yamamoto, H.
Yoshida, S.
Zaleski, K. D.
Zanolin, M.
Zawischa, I.
Zhang, L. ORCID icon
Zhu, R.
Zotov, N.
Zucker, M. ORCID icon
Zweizig, J. ORCID icon
Akutsu, T.
Akutsu, T.
Ando, M
Arai, K. ORCID icon
Araya, A.
Asada, H.
Aso, Y.
Beyersdorf, P.
Fujiki, Y.
Fujimoto, M.-K.
Fujita, R.
Fukushima, M.
Futamase, T.
Hamuro, Y.
Haruyama, T.
Hayama, K.
Iguchi, H.
Iida, Y.
Ioka, K.
Ishitsuka, H.
Kamikubota, N.
Kanda, N.
Kaneyama, T.
Karasawa, Y.
Kasahara, K.
Kasai, T.
Katsuki, M.
Kawamura, S.
Kawamura, M.
Kawazoe, F.
Kojima, Y.
Kokeyama, K.
Kondo, K.
Kozai, Y.
Kudoh, H.
Kuroda, K.
Kuwabara, T.
Matsuda, N.
Mio, N
Miura, K.
Miyama, S.
Miyoki, S.
Mizusawa, H.
Moriwaki, S.
Musha, M.
Nagayama, Y.
Nakagawa, K.
Nakamura, T.
Nakano, H.
Nakao, K.
Nishi, Y.
Numata, K
Ogawa, Y.
Ohashi, M.
Ohishi, N.
Okutomi, A.
Oohara, K.
Otsuka, S.
Saito, Y.
Sakata, S.
Sasaki, M.
Sato, N.
Sato, S.
Sato, Y.
Sato, K.
Sekido, A.
Seto, N.
Shibata, M.
Shinkai, H.
Shintomi, T.
Soida, K.
Somiya, K.
Suzuki, T.
Tagoshi, H.
Takahashi, H.
Takahashi, R.
Takamori, A.
Takemoto, S.
Takeno, K
Tanaka, T.
Taniguchi, K.
Tanji, T.
Tatsumi, D.
Telada, S.
Tokunari, M.
Tomaru, T.
Tsubono, K.
Tsuda, N.
Tsunesada, Y.
Uchiyama, T.
Ueda, K.
Ueda, A, A.
Waseda, K.
Yamamoto, A.
Yamamoto, K.
Yamazaki, T.
Yanagi, Y.
Yokoyama, J.
Yoshida, T.
Zhu, Z.-H
Weinstein, Alan J. ORCID icon
LIGO Scientific Collaboration

Abstract

We search for coincident gravitational wave signals from inspiralling neutron star binaries using LIGO and TAMA300 data taken during early 2003. Using a simple trigger exchange method, we perform an intercollaboration coincidence search during times when TAMA300 and only one of the LIGO sites were operational. We find no evidence of any gravitational wave signals. We place an observational upper limit on the rate of binary neutron star coalescence with component masses between 1 and 3Mסּ of 49 per year per Milky Way equivalent galaxy at a 90% confidence level. The methods developed during this search will find application in future network inspiral analyses.

Additional Information

© 2006 The American Physical Society. Received 11 January 2006; published 16 May 2006. 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. TAMA research is supported by a Grant-in- Aid for Scientific Research on Priority Areas (415) of the Ministry of Education, Culture, Sports, Science and Technology of Japan. This work was also supported in part by JSPS Grant-in-Aid for Scientific Research Nos. 14047214 and 12640269. PACS: 95.85.Sz; 04.80.Nn; 07.05.Kf; 95.55.Ym

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