Search for High Frequency Gravitational-wave Bursts in the First Calendar Tear of LIGO's Fifth Science Run

Authors

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 UniversityFollow

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.

Journal Title

Physical Review D - Particles, Fields, Gravitation and Cosmology

Volume

80

Issue

10

DOI

https://doi.org/10.1103/PhysRevD.80.102002

First Department

Physics

Recommended Citation

Abbott, B. P.; Abbott, R.; Adhikari, R.; Ajith, P.; Allen, B.; Allen, G.; Amin, R. S.; Anderson, S. B.; Anderson, W. G.; Arain, M. A.; Araya, M.; Armandula, H.; Armor, P.; Aso, Y.; Aston, S.; Aufmuth, P.; Aulbert, C.; Babak, S.; Baker, P.; Ballmer, S.; Barker, C.; Barker, D.; Barr, B.; Barriga, P.; Barsotti, L.; Barton, M. A.; Bartos, I.; Bassiri, R.; Bastarrika, M.; Behnke, B.; Benacquista, M.; and Summerscales, Tiffany Z., "Search for High Frequency Gravitational-wave Bursts in the First Calendar Tear of LIGO's Fifth Science Run" (2009). Faculty Publications. 2006.
https://digitalcommons.andrews.edu/pubs/2006

Acknowledgements

Retrieved March 5, 2021 from https://arxiv.org/pdf/0904.4910.pdf