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https://hdl.handle.net/2440/69885
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dc.contributor.author | Ottaway, D. | - |
dc.contributor.author | Fritschel, P. | - |
dc.contributor.author | Waldman, S. | - |
dc.date.issued | 2012 | - |
dc.identifier.citation | Optics Express, 2012; 20(8):8329-8336 | - |
dc.identifier.issn | 1094-4087 | - |
dc.identifier.issn | 1094-4087 | - |
dc.identifier.uri | http://hdl.handle.net/2440/69885 | - |
dc.description.abstract | Second generation gravitational wave detectors are being installed in a number of locations globally. These long-baseline, Michelson interferometers increase the sensitivity between 10 and 40 Hz by many orders of magnitude compared with first generation instruments. Control of non-linear noise coupling from scattered light fields is critical to achieve low frequency performance. In this paper we investigate the requirements on the attenuation of scattered light using a novel time-domain analysis and two years of seismic data from the LIGO Livingston Observatory. | - |
dc.description.statementofresponsibility | David J Ottaway, Peter Fritschel, and Samuel J. Waldman | - |
dc.language.iso | en | - |
dc.publisher | Optical Soc Amer | - |
dc.rights | © 2012 Optical Society of America | - |
dc.source.uri | http://dx.doi.org/10.1364/oe.20.008329 | - |
dc.title | The impact of upconverted scattered light on advanced interferometric gravitational wave detectors | - |
dc.type | Journal article | - |
dc.identifier.doi | 10.1364/OE.20.008329 | - |
pubs.publication-status | Published | - |
dc.identifier.orcid | Ottaway, D. [0000-0001-6794-1591] | - |
Appears in Collections: | Aurora harvest 5 IPAS publications |
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