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Please use this identifier to cite or link to this item: https://hdl.handle.net/2440/116533
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dc.contributor.authorAbbott, B.-
dc.contributor.authorAbbott, R.-
dc.contributor.authorAbbott, T.-
dc.contributor.authorAbernathy, M.-
dc.contributor.authorAckley, K.-
dc.contributor.authorAdams, C.-
dc.contributor.authorAddesso, P.-
dc.contributor.authorAdhikari, R.-
dc.contributor.authorAdya, V.-
dc.contributor.authorAffeldt, C.-
dc.contributor.authorAggarwal, N.-
dc.contributor.authorAguiar, O.-
dc.contributor.authorAin, A.-
dc.contributor.authorAjith, P.-
dc.contributor.authorAllen, B.-
dc.contributor.authorAltin, P.-
dc.contributor.authorAnderson, S.-
dc.contributor.authorAnderson, W.-
dc.contributor.authorArai, K.-
dc.contributor.authorAraya, M.-
dc.contributor.authoret al.-
dc.date.issued2017-
dc.identifier.citationClassical and Quantum Gravity, 2017; 34(4):044001-1-044001-18-
dc.identifier.issn0264-9381-
dc.identifier.issn1361-6382-
dc.identifier.urihttp://hdl.handle.net/2440/116533-
dc.description.abstractThe second-generation of gravitational-wave detectors are just starting operation, and have already yielding their first detections. Research is now concentrated on how to maximize the scientific potential of gravitationalwave astronomy. To support this effort, we present here design targets for a new generation of detectors, which will be capable of observing compact binary sources with high signal-to-noise ratio throughout the Universe.-
dc.description.statementofresponsibilityB P Abbott ... W Kim ... E J King ... J Munch ... D J Ottaway ... P J Veitch ... et al.-
dc.language.isoen-
dc.publisherIOP Publishing Ltd-
dc.rights© 2017 IOP Publishing Ltd-
dc.source.urihttp://dx.doi.org/10.1088/1361-6382/aa51f4-
dc.subjectGravitational waves; cosmic explorer; LIGO-
dc.titleExploring the sensitivity of next generation gravitational wave detectors-
dc.typeJournal article-
dc.identifier.doi10.1088/1361-6382/aa51f4-
dc.relation.grantPHY-0823459-
pubs.publication-statusPublished-
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IPAS publications

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