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dc.contributor.author이현규-
dc.date.accessioned2017-02-16T06:28:30Z-
dc.date.available2017-02-16T06:28:30Z-
dc.date.issued2015-06-
dc.identifier.citationCLASSICAL AND QUANTUM GRAVITY, v. 32, NO 11, Page. 1-2en_US
dc.identifier.issn0264-9381-
dc.identifier.issn1361-6382-
dc.identifier.urihttp://iopscience.iop.org/article/10.1088/0264-9381/32/11/115012/meta-
dc.identifier.urihttp://hdl.handle.net/20.500.11754/25552-
dc.description.abstractIn 2009-2010, the Laser Interferometer Gravitational-Wave Observatory (LIGO) operated together with international partners Virgo and GEO600 as a network to search for gravitational waves (GWs) of astrophysical origin. The sensitivity of these detectors was limited by a combination of noise sources inherent to the instrumental design and its environment, often localized in time or frequency, that couple into the GW readout. Here we review the performance of the LIGO instruments during this epoch, the work done to characterize the detectors and their data, and the effect that transient and continuous noise artefacts have on the sensitivity of LIGO to a variety of astrophysical sources.en_US
dc.description.sponsorshipThe authors gratefully acknowledge the support of the United States National Science Foundation for the construction and operation of the LIGO Laboratory, 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, and the Italian Istituto Nazionale di Fisica Nucleare and the French Centre National de la Recherche Scientifique for the construction and operation of the Virgo detector. The authors also gratefully acknowledge the support of the research by these agencies and by the Australian Research Council, the International Science Linkages program of the Commonwealth of Australia, the Council of Scientific and Industrial Research of India, the Istituto Nazionale di Fisica Nucleare of Italy, the Spanish Ministerio de Economia y Competitividad, the Conselleria d'Economia Hisenda i Innovacio of the Govern de les Illes Balears, the Foundation for Fundamental Research on Matter supported by the Netherlands Organization for Scientific Research, the Polish Ministry of Science and Higher Education, the FOCUS Programme of Foundation for Polish Science, the Royal Society, the Scottish Funding Council, the Scottish Universities Physics Alliance, The National Aeronautics and Space Administration, the National Research Foundation of Korea, Industry Canada and the Province of Ontario through the Ministry of Economic Development and Innovation, the National Science and Engineering Research Council Canada, the Carnegie Trust, the Leverhulme Trust, the David and Lucile Packard Foundation, the Research Corporation, and the Alfred P Sloan Foundation.en_US
dc.language.isoenen_US
dc.publisherIOP PUBLISHING LTDen_US
dc.subjectLIGOen_US
dc.subjectgravitational wavesen_US
dc.subjectdetector characterizationen_US
dc.titleCharacterization of the LIGO detectors during their sixth science runen_US
dc.typeArticleen_US
dc.relation.no11-
dc.relation.volume32-
dc.identifier.doi10.1088/0264-9381/32/11/115012-
dc.relation.page1-2-
dc.relation.journalCLASSICAL AND QUANTUM GRAVITY-
dc.contributor.googleauthorAasi, J.-
dc.contributor.googleauthorAbadie, J.-
dc.contributor.googleauthorAbbott, B. P.-
dc.contributor.googleauthorAbbott, R.-
dc.contributor.googleauthorAbbott, T-
dc.contributor.googleauthorAbernathy, M. R.-
dc.contributor.googleauthorAccadia, T.-
dc.contributor.googleauthorAcernese, F.-
dc.contributor.googleauthorAdams, C.-
dc.contributor.googleauthorLee, H. K.-
dc.relation.code2015000505-
dc.sector.campusS-
dc.sector.daehakCOLLEGE OF NATURAL SCIENCES[S]-
dc.sector.departmentDEPARTMENT OF PHYSICS-
dc.identifier.pidhyunkyu-
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COLLEGE OF NATURAL SCIENCES[S](자연과학대학) > PHYSICS(물리학과) > Articles
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