Published January 21, 2004
| Submitted
Journal Article
Open
Detector description and performance for the first coincidence observations between LIGO and GEO
- Creators
- Abbott, B.
- Ageev, A.
- Anderson, S. B.
- Araya, M.
- Armandula, H.
- Asiri, F.
- Barish, B. C.
- Barnes, M.
- Barton, M. A.
- Bhawal, B.
- Bilenko, I. A.
-
Billingsley, G.
- Black, E.
- Blackburn, K.
- Bogue, L.
- Bork, R.
- Braginsky, V. B.
- Busby, D.
- Cardenas, L.
- Chandler, A.
- Chapsky, J.
- Charlton, P.
-
Coyne, D.
- Creighton, T. D.
- D'Ambrosio, E.
- DeSalvo, R.
- Ding, H.
- Edlund, J.
- Ehrens, P.
- Etzel, T.
- Evans, M.
- Farnham, D.
- Fine, M.
- Gillespie, A.
- Grimmett, D.
- Hartunian, A.
- Heefner, J.
- Hoang, P.
- Hrynevych, M.
- Ivanov, A.
- Jones, L.
- Jungwirth, D.
- Kells, W.
- King, C.
- King, P.
-
Kozak, D.
- Lazzarini, A.
- Lei, M.
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Libbrecht, K.
- Lindquist, P.
- Liu, S.
- Logan, J.
- Lyons, T. T.
- Mageswaran, M.
- Mailand, K.
- Majid, W.
- Mann, F.
- Márka, S.
- Maros, E.
- Mason, J.
- Meshkov, S.
- Miyakawa, O.
- Miyoki, S.
- Mours, B.
- Nocera, F.
- Ouimette, D.
- Pedraza, M.
- Rao, S. R.
- Redding, D.
- Regehr, M. W.
- Reilly, K. T.
- Reithmaier, K.
- Robison, L.
- Romie, J.
- Rose, D.
- Russell, P.
- Salzman, I.
- Sanders, G. H.
- Sannibale, V.
- Schmidt, V.
- Sears, B.
- Seel, S.
- Shawhan, P.
- Sievers, L.
- Smith, M. R.
- Spero, R.
- Sumner, M. C.
- Sylvestre, J.
- Takamori, A.
- Tariq, H.
- Taylor, R.
- Tilav, S.
- Torrie, C.
- Tyler, W.
- Vass, S.
- Wallace, L.
- Ware, B.
- Webber, D.
-
Weinstein, A. J.
- Wen, L.
- Whitcomb, S. E.
- Willems, P. A.
- Wilson, A.
- Yamamoto, H.
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Zhang, L.
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Zweizig, J.
- Buonanno, A.
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Chen, Y.
- Thorne, K. S.
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Vallisneri, M.
- Drever, R. W. P.
-
Tinto, M.
-
Williams, R.
- LIGO Scientific Collaboration
Chicago
Abstract
For 17 days in August and September 2002, the LIGO and GEO interferometer gravitational wave detectors were operated in coincidence to produce their first data for scientific analysis. Although the detectors were still far from their design sensitivity levels, the data can be used to place better upper limits on the flux of gravitational waves incident on the earth than previous direct measurements. This paper describes the instruments and the data in some detail, as a companion to analysis papers based on the first data.
Additional Information
© 2003 Elsevier B.V. Received 30 September 2003. 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 their 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 Ciencia y Tecnologia, the John Simon Guggenheim Foundation, the David and Lucile Packard Foundation, the Research Corporation, and the Alfred P. Sloan Foundation. This paper has been assigned LIGO Laboratory document number LIGO-P030024.Attached Files
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Additional details
- Eprint ID
- 43290
- Resolver ID
- CaltechAUTHORS:20140109-094808747
- NSF
- Max-Planck-Society
- State of Niedersachsen/Germany
- Australian Research Council
- Natural Sciences and Engineering Research Council of Canada (NSERC)
- Council of Scientific and Industrial Research (India)
- Department of Science and Technology (India)
- Ministerio de Ciencia y Tecnologia (MCYT)
- John Simon Guggenheim Foundation
- David and Lucile Packard Foundation
- Research Corporation
- Alfred P. Sloan Foundation
- Created
-
2014-01-10Created from EPrint's datestamp field
- Updated
-
2021-11-10Created from EPrint's last_modified field
- Caltech groups
- LIGO
- Other Numbering System Name
- LIGO Document
- Other Numbering System Identifier
- LIGO-P030024