Search for gravitational waves from compact binary coalescence in LIGO and Virgo data from S5 and VSR1

被引:144
作者
Abadie, J. [1 ]
Abbott, B. P. [1 ]
Abbott, R. [1 ]
Abernathy, M. [85 ]
Accadia, T. [37 ]
Acernese, F. [20 ,21 ,22 ]
Adams, C. [40 ]
Adhikari, R. [1 ]
Ajith, P. [1 ]
Allen, B. [97 ]
Allen, G. [71 ]
Ceron, E. Amador [97 ]
Amin, R. S. [43 ]
Anderson, S. B. [1 ]
Anderson, W. G. [97 ]
Antonucci, F. [28 ,29 ]
Arain, M. A. [84 ]
Araya, M. [1 ]
Aronsson, M. [1 ]
Arun, K. G. [35 ,36 ]
Aso, Y. [1 ]
Aston, S. [83 ]
Astone, P. [28 ,29 ]
Atkinson, D. E. [39 ]
Aufmuth, P. [38 ]
Aulbert, C. [3 ]
Babak, S. [2 ]
Baker, P. [46 ]
Ballardin, G. [13 ]
Ballinger, T. [10 ]
Ballmer, S. [1 ]
Barker, D. [39 ]
Barnum, S. [67 ]
Barone, F. [20 ,21 ,22 ]
Barr, B. [85 ]
Barriga, P. [96 ]
Barsotti, L. [41 ]
Barsuglia, M. [5 ]
Barton, M. A. [39 ]
Bartos, I. [12 ]
Bassiri, R. [85 ]
Bastarrika, M. [85 ]
Bauchrowitz, J. [3 ]
Bauer, Th. S. [50 ]
Behnke, B. [2 ]
Beker, M. G. [50 ]
Belletoile, A. [37 ,97 ]
Benacquista, M. [78 ]
Bertolini, A. [3 ]
Betzwieser, J. [1 ]
机构
[1] CALTECH, LIGO, Pasadena, CA 91125 USA
[2] Max Planck Inst Gravitat Phys, Albert Einstein Inst, D-14476 Golm, Germany
[3] Max Planck Inst Gravitat Phys, Albert Einstein Inst, D-30167 Hannover, Germany
[4] Andrews Univ, Berrien Springs, MI 49104 USA
[5] Univ Denis Diderot Paris 7, Observ Paris, CEA, CNRS,UMR7164,IN2P3,DSM,IRFU, Paris, France
[6] Australian Natl Univ, Canberra, ACT 0200, Australia
[7] Calif State Univ Fullerton, Fullerton, CA 92831 USA
[8] Caltech CaRT, Pasadena, CA 91125 USA
[9] Cardiff Univ, Cardiff CF24 3AA, S Glam, Wales
[10] Carleton Coll, Northfield, MN 55057 USA
[11] Charles Sturt Univ, Wagga Wagga, NSW 2678, Australia
[12] Columbia Univ, New York, NY 10027 USA
[13] European Gravitat Observ, I-56021 Cascina, PI, Italy
[14] Embry Riddle Aeronaut Univ, Prescott, AZ 86301 USA
[15] Eotvos Lorand Univ, H-1053 Budapest, Hungary
[16] Hobart & William Smith Coll, Geneva, NY 14456 USA
[17] Ist Nazl Fis Nucl, Sez Firenze, I-50019 Sesto Fiorentino, Italy
[18] Univ Urbino Carlo Bo, I-61029 Urbino, Italy
[19] Ist Nazl Fis Nucl, Sez Genova, I-16146 Genoa, Italy
[20] Ist Nazl Fis Nucl, Sez Napoli, I-80126 Naples, Italy
[21] Univ Naples Federico II, I-80126 Naples, Italy
[22] Univ Salerno, I-84084 Salerno, Italy
[23] Ist Nazl Fis Nucl, Sez Perugia, I-06123 Perugia, Italy
[24] Univ Perugia, I-06123 Perugia, Italy
[25] Ist Nazl Fis Nucl, Sez Pisa, I-56127 Pisa, Italy
[26] Univ Pisa, I-56127 Pisa, Italy
[27] Univ Siena, I-53100 Siena, Italy
[28] Ist Nazl Fis Nucl, Sez Roma, I-00185 Rome, Italy
[29] Univ Roma La Sapienza, I-00185 Rome, Italy
[30] Univ Roma Tor Vergata, I-00133 Rome, Italy
[31] Ist Nazl Fis Nucl, Sez Roma, I-00133 Rome, Italy
[32] Univ Aquila, I-67100 Laquila, Italy
[33] Inst Appl Phys, Nizhnii Novgorod 603950, Russia
[34] Interuniv Ctr Astron & Astrophys, Pune 411007, Maharashtra, India
[35] Univ Paris Sud, LAL, IN2P3, CNRS, F-91898 Orsay, France
[36] CNRS, ESPCI, F-75005 Paris, France
[37] Univ Savoie, Lab Annecy Le Vieux Phys Particules, CNRS, IN2P3, F-74941 Annecy Le Vieux, France
[38] Leibniz Univ Hannover, D-30167 Hannover, Germany
[39] LIGO Hanford Observ, Richland, WA 99352 USA
[40] LIGO Livingston Observ, Livingston, LA 70754 USA
[41] MIT, LIGO, Cambridge, MA 02139 USA
[42] CNRS, IN2P3, LMA, F-69622 Villeurbanne, France
[43] Louisiana State Univ, Baton Rouge, LA 70803 USA
[44] Louisiana Tech Univ, Ruston, LA 71272 USA
[45] McNeese State Univ, Lake Charles, LA 70609 USA
[46] Montana State Univ, Bozeman, MT 59717 USA
[47] Moscow MV Lomonosov State Univ, Moscow 119992, Russia
[48] NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA
[49] Natl Astron Observ Japan, Tokyo 1818588, Japan
[50] NIKHEF, Natl Inst Subatom Phys, NL-1009 DB Amsterdam, Netherlands
来源
PHYSICAL REVIEW D | 2010年 / 82卷 / 10期
基金
美国国家科学基金会; 美国国家航空航天局; 澳大利亚研究理事会;
关键词
FORMS;
D O I
10.1103/PhysRevD.82.102001
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We report the results of the first search for gravitational waves from compact binary coalescence using data from the Laser Interferometer Gravitational-Wave Observatory and Virgo detectors. Five months of data were collected during the Laser Interferometer Gravitational-Wave Observatory's S5 and Virgo's VSR1 science runs. The search focused on signals from binary mergers with a total mass between 2 and 35M(circle dot). No gravitational waves are identified. The cumulative 90%-confidence upper limits on the rate of compact binary coalescence are calculated for nonspinning binary neutron stars, black hole-neutron star systems, and binary black holes to be 8: 7 X 10(-3) yr(-1) L-10(-1), 2.2 X 10(-3) yr(-1) L-10(-1), and 4.4 X 10(-4) yr(-1) L-10(-1), respectively, where L-10 is 10(10) times the blue solar luminosity. These upper limits are compared with astrophysical expectations.
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页数:11
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