Please use this identifier to cite or link to this item: http://hdl.handle.net/2440/48830
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Type: Journal article
Title: Detector description and performance for the first coincidence observations between LIGO and GEO
Author: Abbott, B.
Acernese, F.
Adhikari, R.
Allen, B.
Amin, R.
Anderson, S.
Anderson, W.
Araya, M.
Armandula, H.
Asiri, F.
Aufmuth, P.
Aulbert, C.
Babak, S.
Balasubramanian, R.
Ballmer, S.
Barish, B.
Barker, D.
Barker, C.
Barnes, M.
Barr, B.
et al.
Citation: Nuclear Instruments & Methods in Physics Research Section A-accelerators Spectrometers Detectors and Associated Equipment, 2004; 517(1-3):154-179
Publisher: Elsevier Science BV
Issue Date: 2004
ISSN: 0168-9002
Statement of
Responsibility: 
B. Abbott...C. Killow...D. Ottaway...et al.
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.
Keywords: LIGO; Gravitational wave; Interferometer; Observatory
Rights: © 2003 Elsevier B.V. All rights reserved.
RMID: 0020083093
DOI: 10.1016/j.nima.2003.11.124
Appears in Collections:Physics publications

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