Published March 7, 2008
| Submitted + Published
Journal Article
Open
Search for gravitational waves from binary inspirals in S3 and S4 LIGO data
- Creators
- Abbott, B.
- Drever, R. W. P.
-
Brown, D. A.
- Savov, P.
- Thorne, K. S.
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Vallisneri, M.
- Abbott, R.
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Adhikari, Rana X.
- Agresti, J.
- Anderson, S. B.
- Araya, M.
- Armandula, H.
- Ballmer, S.
- Barish, B. C.
- Bhawal, B.
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Billingsley, G.
- Black, E.
- Blackburn, K.
- Bork, R.
- Boschi, V.
- Busby, D.
- Cardenas, L.
- Cepeda, C.
- Chatterji, S.
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Coyne, D.
- Creighton, T. D.
- D'Ambrosio, E.
- De Salvo, R.
- Dupuis, R. J.
- Ehrens, P.
- Espinoza, E.
- Etzel, T.
- Evans, M.
- Fairhurst, S.
- Fazi, D.
- Goggin, L.
- Heefner, J.
- Ivanov, A.
- Kells, W.
- Keppel, D. G.
- King, P.
- Kondrashov, V.
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Kozak, D.
- Lazzarini, A.
- Lei, M.
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Libbrecht, K.
- Lindquist, P.
- Mageswaran, M.
- Mailand, K.
- Mandic, V.
- Maros, E.
- Marx, J. N.
- Meshkov, S.
- Messaritaki, E.
- Meyers, D.
- Miyakawa, O.
- Nash, T.
- Nocera, F.
- Patel, P.
- Pedraza, M.
- Robertson, N. A.
- Russell, P.
- Samidi, M.
- Sanders, G. H.
- Sannibale, V.
- Sears, B.
- Smith, M. R.
- Sutton, P. J.
- Tarallo, M.
- Taylor, R.
- Tyler, W.
- Varvella, M.
- Vass, S.
- Villar, A.
- Waldman, S. J.
- Wallace, L.
- Ward, R.
- Webber, D.
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Weinstein, A. J.
- Whitcomb, S. E.
- Willems, P. A.
- Yamamoto, H.
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Zhang, L.
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Zweizig, J.
- LIGO Scientific Collaboration
Abstract
We report on a search for gravitational waves from the coalescence of compact binaries during the third and fourth LIGO science runs. The search focused on gravitational waves generated during the inspiral phase of the binary evolution. In our analysis, we considered three categories of compact binary systems, ordered by mass: (i) primordial black hole binaries with masses in the range 0.35M_⊙
Additional Information
© 2008 The American Physical Society. Received 26 April 2007; published 7 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 Science and Technology Facilities 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 Council of Scientific and Industrial Research of India, the Istituto Nazionale di Fisica Nucleare of Italy, the Spanish Ministerio de Educaciόn y Ciencia, the Conselleria d'Economia, Hisenda i Innovaciό of the Govern de les Illes Balears, the Scottish Funding Council, the Scottish Universities Physics Alliance, The National Aeronautics and Space Administration, the Carnegie Trust, the Leverhulme Trust, the David and Lucile Packard Foundation, the Research Corporation, and the Alfred P. Sloan Foundation.Attached Files
Published - PhysRevD.77.062002.pdf
Submitted - 0704.3368v4.pdf
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Additional details
- Eprint ID
- 44559
- Resolver ID
- CaltechAUTHORS:20140401-081124003
- NSF
- Science and Technology Facilities Council (STFC)
- Max-Planck-Society
- Australian Research Council
- Council of Scientific and Industrial Research (India)
- Istituto Nazionale di Fisica Nucleare (INFN)
- Ministerio de Educaciόn y Ciencia (MEC)
- Scottish Funding Council
- Scottish Universities Physics Alliance
- NASA
- Carnegie Trust
- Leverhulme Trust
- David and Lucile Packard Foundation
- Research Corporation
- Alfred P. Sloan Foundation
- Conselleria d'Economia, Hisenda i Innovaciό of the Govern de les Illes Balears
- Created
-
2014-04-01Created from EPrint's datestamp field
- Updated
-
2021-11-10Created from EPrint's last_modified field
- Caltech groups
- LIGO