Paper abstract bibtex

We present the results of a search for short-duration gravitational-wave bursts associated with 39 gamma-ray bursts (GRBs) detected by gamma-ray satellite experiments during LIGO?s S2, S3, and S4 science runs. The search involves calculating the crosscorrelation between two interferometer data streams surrounding the GRB trigger time. We search for associated gravitational radiation from single GRBs, and also apply statistical tests to search for a gravitational-wave signature associated with the whole sample. For the sample examined, we find no evidence for the association of gravitational radiation with GRBs, either on a single-GRB basis or on a statistical basis. Simulating gravitational-wave bursts with sine-Gaussian waveforms, we set upper limits on the root-sum-square of the gravitational-wave strain amplitude of such waveforms at the times of the GRB triggers. We also demonstrate how a sample of several GRBs can be used collectively to set constraints on population models. The small number of GRBs and the significant change in sensitivity of the detectors over the three runs, however, limits the usefulness of a population study for the S2, S3, and S4 runs. Finally, we discuss prospects for the search sensitivity for the ongoing S5 run, and beyond for the next generation of detectors.

@article{caltechauthors45892, volume = {77}, number = {6}, month = {March}, author = {B. Abbott and R. W. P. Drever and M. Tinto and D. A. Brown and P. Savov and X. Siemens and K. S. Thorne and M. Vallisneri and R. Abbott and R. Adhikari and J. Agresti and S. B. Anderson and M. Araya and H. Armandula and S. Ballmer and B. C. Barish and B. Bhawal and G. Billingsley and E. Black and K. Blackburn and R. Bork and V. Boschi and D. Busby and L. Cardenas and C. Cepeda and S. Chatterji and D. Coyne and T. D. Creighton and E. D'Ambrosio and R. DeSalvo and H. Ding and R. J. Dupuis and P. Ehrens and E. Espinoza and T. Etzel and M. Evans and S. Fairhurst and D. Fazi and L. Goggin and J. Heefner and A. Ivanov and W. Kells and D. G. Keppel and P. King and V. Kondrashov and D. Kozak and A. Lazzarini and M. Lei and K. Libbrecht and P. Lindquist and J. Logan and M. Mageswaran and K. Mailand and V. Mandic and E. Maros and J. N. Marx and S. Meshkov and E. Messaritaki and D. Meyers and O. Miyakawa and T. Nash and F. Nocera and P. Patel and M. Pedraza and N. A. Robertson and P. Russell and M. Samidi and G. H. Sanders and V. Sannibale and B. Sears and M. R. Smith and P. J. Sutton and J. Sylvestre and A. Takamori and M. Tarallo and R. Taylor and W. Tyler and M. Varvella and S. Vass and A. Villar and S. J. Waldman and L. Wallace and R. Ward and D. Webber and A. J. Weinstein and S. E. Whitcomb and P. A. Willems and H. Yamamoto and L. Zhang and J. Zweizig}, note = {{\copyright} 2008 The American Physical Society. Received 16 October 2007; published 17 March 2008. 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 National Aeronautics and Space Administration, the John Simon Guggenheim Foundation, the Alexander von Humboldt Foundation, the Leverhulme Trust, the David and Lucile Packard Foundation, the Research Corporation, and the Alfred P. Sloan Foundation. This document has been assigned LIGO Laboratory document number LIGOP060024-07-Z.}, title = {Search for gravitational waves associated with 39 gamma-ray bursts using data from the second, third, and fourth LIGO runs}, publisher = {American Physical Society}, year = {2008}, journal = {Physical Review D}, pages = {Art. No. 062004}, url = {http://resolver.caltech.edu/CaltechAUTHORS:20140522-133958402}, abstract = {We present the results of a search for short-duration gravitational-wave bursts associated with 39 gamma-ray bursts (GRBs) detected by gamma-ray satellite experiments during LIGO?s S2, S3, and S4 science runs. The search involves calculating the crosscorrelation between two interferometer data streams surrounding the GRB trigger time. We search for associated gravitational radiation from single GRBs, and also apply statistical tests to search for a gravitational-wave signature associated with the whole sample. For the sample examined, we find no evidence for the association of gravitational radiation with GRBs, either on a single-GRB basis or on a statistical basis. Simulating gravitational-wave bursts with sine-Gaussian waveforms, we set upper limits on the root-sum-square of the gravitational-wave strain amplitude of such waveforms at the times of the GRB triggers. We also demonstrate how a sample of several GRBs can be used collectively to set constraints on population models. The small number of GRBs and the significant change in sensitivity of the detectors over the three runs, however, limits the usefulness of a population study for the S2, S3, and S4 runs. Finally, we discuss prospects for the search sensitivity for the ongoing S5 run, and beyond for the next generation of detectors.} }

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