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|a (TOE)ost1847796
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|a E 1.99: arxiv:gr-qc/0308043
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|a Detector description and performance for the first coincidence observations between LIGO and GEO
|h [electronic resource]
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|a Washington, D.C. :
|b United States. Department of Energy. Office of High Energy Physics ;
|a Oak Ridge, Tenn. :
|b Distributed by the Office of Scientific and Technical Information, U.S. Department of Energy,
|c 2003.
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|a Size: 154 :
|b digital, PDF file.
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|a Published through Scitech Connect.
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|a 08/01/2003.
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|a "fermilab-pub-03-458."
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|a " arxiv:gr-qc/0308043."
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|a "Other: oai:inspirehep.net:625917."
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|a Abbott, B.; et al.;
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|a 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.
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|a 46 instrumentation related to nuclear science and technology
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|a Fermi National Accelerator Laboratory.
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|a United States. Department of Energy. Office of High Energy Physics.
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|a United States.
|b Department of Energy.
|b Office of Scientific and Technical Information
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|u https://www.osti.gov/servlets/purl/1847796
|z Full Text (via OSTI)
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