Characterization of the LIGO detectors during their sixth science run
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Abstract
In 2009-2010, the Laser Interferometer Gravitational-Wave Observatory \n(LIGO) operated together with international partners Virgo and GEO600 as \na network to search for gravitational waves (GWs) of astrophysical \norigin. The sensitivity of these detectors was limited by a combination \nof noise sources inherent to the instrumental design and its \nenvironment, often localized in time or frequency, that couple into the \nGW readout. Here we review the performance of the LIGO instruments \nduring this epoch, the work done to characterize the detectors and their \ndata, and the effect that transient and continuous noise artefacts have \non the sensitivity of LIGO to a variety of astrophysical sources.
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The record
- Venue
- Classical and Quantum Gravity
- Topic
- Pulsars and Gravitational Waves Research
- Field
- Physics and Astronomy
- Canadian institutions
- Canadian Institute for Theoretical AstrophysicsPerimeter InstituteUniversity of Toronto
- Funders
- Division of PhysicsMinistero dello Sviluppo EconomicoAustralian Research CouncilNational Research Foundation of KoreaMinisterio de Economía y CompetitividadCentre National de la Recherche ScientifiqueIndustry CanadaGovern de les Illes BalearsFundacja na rzecz Nauki PolskiejNational Science FoundationRoyal SocietyScottish Funding CouncilScottish Universities Physics AllianceIstituto Nazionale di Fisica NucleareDavid and Lucile Packard FoundationHungarian Scientific Research FundLeverhulme TrustNederlandse Organisatie voor Wetenschappelijk OnderzoekCouncil of Scientific and Industrial Research, IndiaScience and Technology Facilities CouncilNational Research FoundationAlfred P. Sloan FoundationNational Aeronautics and Space Administration
- Keywords
- LIGOPhysicsGravitational waveInterferometryDetectorNoise (video)AstronomyAstrophysicsSensitivity (control systems)Gravitational-wave astronomyOpticsElectronic engineeringComputer science
- Has abstract in OpenAlex
- yes