Search for high frequency gravitational-wave bursts in the first calendar year of LIGO's fifth science run
Author(s)
Wipf, Christopher C.; Weiss, Rainer; Waldman, Samuel J.; Villadsen, J.; Stein, Leo Chaim; Stein, Andrew J.; Smith, Nicolas de Mateo; Shapiro, B.; Sarin, P.; Mavalvala, Nergis; Markowitz, Jared John; Katsavounidis, Erotokritos; Hughey, Brennan J.; Harry, Gregory; Grimaldi, F.; Goda, K.; Foley, Stephany; Duke, I.; Cao, Junwei; Brunet, G.; Blackburn, Lindy L.; Barsotti, Lisa; MacInnis, Myron E; Fritschel, Peter K; Evans, Matthew J; Donovan, Frederick J; Corbitt, Thomas R; Bodiya, Timothy P.; Zucker, Michael E; Shoemaker, David H; Mittleman, Richard K; Mason, Kenneth R; ... Show more Show less
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Show full item recordAbstract
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 5.4 year[superscript -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.
Date issued
2009-11Department
Massachusetts Institute of Technology. Department of Physics; MIT Kavli Institute for Astrophysics and Space ResearchJournal
Physical Review D
Publisher
American Physical Society
Citation
The LIGO Scientific Collaboration et al. “Search for high frequency gravitational-wave bursts in the first calendar year of LIGO's fifth science run.” Physical Review D 80.10 (2009): 102002. © 2009 The American Physical Society
Version: Final published version
Other identifiers
LIGO Laboratory document No. LIGO-P080080
ISSN
1550-2368
1550-7998