Optimal location of a new interferometric gravitational wave observatory

Antony C. Searle, Susan M. Scott, David E. McClelland, Lee S. Finn

Research output: Contribution to journalArticle

9 Citations (Scopus)

Abstract

As 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.

Original languageEnglish (US)
Article number124014
JournalPhysical Review D - Particles, Fields, Gravitation and Cosmology
Volume73
Issue number12
DOIs
StatePublished - Jun 19 2006

Fingerprint

Optimal Location
Gravitational Waves
Observatory
gravitational waves
observatories
Astronomy
astronomy
Expand
Model
Strategy

All Science Journal Classification (ASJC) codes

  • Nuclear and High Energy Physics
  • Physics and Astronomy (miscellaneous)

Cite this

Searle, Antony C. ; Scott, Susan M. ; McClelland, David E. ; Finn, Lee S. / Optimal location of a new interferometric gravitational wave observatory. In: Physical Review D - Particles, Fields, Gravitation and Cosmology. 2006 ; Vol. 73, No. 12.
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Optimal location of a new interferometric gravitational wave observatory. / Searle, Antony C.; Scott, Susan M.; McClelland, David E.; Finn, Lee S.

In: Physical Review D - Particles, Fields, Gravitation and Cosmology, Vol. 73, No. 12, 124014, 19.06.2006.

Research output: Contribution to journalArticle

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