Characterization of the LIGO detectors during their sixth science run

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dc.contributor.author Sengupta, Anand
dc.date.accessioned 2015-01-18T10:56:15Z
dc.date.available 2015-01-18T10:56:15Z
dc.date.issued 2014-10
dc.identifier.citation Sengupta, Anand et al., “Characterization of the LIGO detectors during their sixth science run”, arXiv, Cornell University Library, DOI: arXiv:1410.7764, Oct. 2014. en_US
dc.identifier.other http://arxiv.org/abs/1410.7764
dc.identifier.uri https://repository.iitgn.ac.in/handle/123456789/1569
dc.description.abstract In 2009-2010, the Laser Interferometer Gravitational-wave Observa- tory (LIGO) operated together with international partners Virgo and GEO600 as a network to search for gravitational waves of astrophysical origin. The sensitiv- ity 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 gravitational-wave readout. Here we review the performance of the LIGO instruments during this epoch, the work done to characterize the de- tectors 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.statementofresponsibility by Anand Sengupta et al.
dc.language.iso en_US en_US
dc.publisher Cornell University Library en_US
dc.subject General Relativity en_US
dc.subject Quantum Cosmology en_US
dc.subject Instrumentation en_US
dc.subject Methods for Astrophysics en_US
dc.title Characterization of the LIGO detectors during their sixth science run en_US
dc.type Preprint en_US


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