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Search for High Frequency Gravitational-wave Bursts in the First Calendar Tear of LIGO's Fifth Science Run
Physical Review D - Particles, Fields, Gravitation and Cosmology
  • B. P. Abbott, California Institute of Technology
  • R. Abbott, California Institute of Technology
  • R. Adhikari, California Institute of Technology
  • P. Ajith, Max Planck Institute for Gravitational Physics (Albert Einstein Institute)
  • B. Allen, Max Planck Institute for Gravitational Physics (Albert Einstein Institute)
  • G. Allen, Stanford University
  • R. S. Amin, Louisiana State University
  • S. B. Anderson, California Institute of Technology
  • W. G. Anderson, University of Wisconsin-Milwaukee
  • M. A. Arain, University of Florida
  • M. Araya, California Institute of Technology
  • H. Armandula, California Institute of Technology
  • P. Armor, University of Wisconsin-Milwaukee
  • Y. Aso, California Institute of Technology
  • S. Aston, University of Birmingham
  • P. Aufmuth, Gottfried Wilhelm Leibniz Universität Hannover
  • C. Aulbert, Max Planck Institute for Gravitational Physics (Albert Einstein Institute)
  • S. Babak, Max Planck Institute for Gravitational Physics (Albert Einstein Institute)
  • P. Baker, Montana State University
  • S. Ballmer, California Institute of Technology
  • C. Barker, LIGO Hanford
  • D. Barker, LIGO Hanford
  • B. Barr, University of Glasgow
  • P. Barriga, The University of Western Australia
  • L. Barsotti, LIGO, Massachusetts Institute of Technology
  • M. A. Barton, California Institute of Technology
  • I. Bartos, Columbia University in the City of New York
  • R. Bassiri, University of Glasgow
  • M. Bastarrika, University of Glasgow
  • B. Behnke, Max Planck Institute for Gravitational Physics (Albert Einstein Institute)
  • M. Benacquista, University of Texas at Brownsville and Texas Southmost College
  • Tiffany Z. Summerscales, Andrews University
Document Type
Article
Publication Date
11-11-2009
Abstract

We present an all-sky search for gravitational waves in the frequency range 1 to 6 kHz during the first calendar year of LIGO's fifth science run. This is the first untriggered LIGO burst analysis to be conducted above 3 kHz. We discuss the unique properties of interferometric data in this regime. 161.3 days of triple-coincident data were analyzed. No gravitational events above threshold were observed and a frequentist upper limit of 5.4year-1 on the rate of strong gravitational-wave bursts was placed at a 90% confidence level. Implications for specific theoretical models of gravitational-wave emission are also discussed. © 2009 The American Physical Society.

DOI
https://doi.org/10.1103/PhysRevD.80.102002
First Department
Physics
Acknowledgements
Retrieved March 5, 2021 from https://arxiv.org/pdf/0904.4910.pdf
Citation Information
B. P. Abbott, R. Abbott, R. Adhikari, P. Ajith, et al.. "Search for High Frequency Gravitational-wave Bursts in the First Calendar Tear of LIGO's Fifth Science Run" Physical Review D - Particles, Fields, Gravitation and Cosmology Vol. 80 Iss. 10 (2009)
Available at: http://works.bepress.com/tiffany_summerscales/209/