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Optimal location of a new interferometric gravitational wave observatory

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dc.contributor.authorSearle, Antony
dc.contributor.authorScott, Susan M
dc.contributor.authorMcClelland, David
dc.contributor.authorFinn, Lee
dc.date.accessioned2015-12-07T22:21:07Z
dc.date.issued2006
dc.date.updated2015-12-07T08:53:58Z
dc.description.abstractAs gravitational wave astronomy becomes a reality, issues of how to best combine and expand the global network of observatories will come to the fore. We have constructed several models to determine optimal additions to an existing global network of observatories for certain gravitational wave source populations and detection strategies.
dc.identifier.issn0556-2821
dc.identifier.urihttp://hdl.handle.net/1885/19891
dc.publisherAmerican Physical Society
dc.sourcePhysical Review D
dc.titleOptimal location of a new interferometric gravitational wave observatory
dc.typeJournal article
local.bibliographicCitation.lastpage10
local.bibliographicCitation.startpage124014/1
local.contributor.affiliationSearle, Antony, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationScott, Susan M, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationMcClelland, David, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationFinn, Lee, Pennsylvania State University
local.contributor.authoruidSearle, Antony, u9719170
local.contributor.authoruidScott, Susan M, u8911327
local.contributor.authoruidMcClelland, David, u8802403
local.description.notesImported from ARIES
local.identifier.absfor020110 - Stellar Astronomy and Planetary Systems
local.identifier.absfor010501 - Algebraic Structures in Mathematical Physics
local.identifier.ariespublicationu4103646xPUB10
local.identifier.citationvolume73
local.identifier.doi10.1103/PhysRevD.73.124014
local.identifier.scopusID2-s2.0-33745032294
local.type.statusPublished Version

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