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Volumn 59, Issue 10, 1999, Pages

Detecting a stochastic background of gravitational radiation: Signal processing strategies and sensitivities

Author keywords

[No Author keywords available]

Indexed keywords


EID: 85037884087     PISSN: 15507998     EISSN: 15502368     Source Type: Journal    
DOI: 10.1103/PhysRevD.59.102001     Document Type: Article
Times cited : (907)

References (32)
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    • K. Danzmann et al., in Gravitational Wave Experiments [2], p. 100.
  • 4
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    • K. Tsubono, in Gravitational Wave Experiments [2], p. 112.
    • K. Tsubono, in Gravitational Wave Experiments [2], p. 112.
  • 11
    • 85037893312 scopus 로고    scopus 로고
    • D.G. Blair, R. Burman, L. Ju, S. Woodings, M. Mulder, and M.G. Zadnik, “The supernova cosmological background of gravitational waves,” report, University of Western Australia, 1997;
    • D.G. Blair, R. Burman, L. Ju, S. Woodings, M. Mulder, and M.G. Zadnik, “The supernova cosmological background of gravitational waves,” report, University of Western Australia, 1997;
  • 20
    • 85037907910 scopus 로고    scopus 로고
    • L.S. Finn, “Gravitational-wave data analysis with multiple detectors: The gravitational-wave receiver. I. Deterministic sources” (in preparation).
    • Finn, L.S.1
  • 21
    • 85037890360 scopus 로고    scopus 로고
    • L.S. Finn, “Gravitational-wave data analysis with multiple detectors: The gravitational-wave receiver. II. Stochastic signals” (in preparation).
    • Finn, L.S.1
  • 26
    • 85037917680 scopus 로고    scopus 로고
    • N. Christensen, Ph.D. thesis, Massachusetts Institute of Technology, 1990.
    • N. Christensen, Ph.D. thesis, Massachusetts Institute of Technology, 1990.
  • 27
    • 85037893534 scopus 로고    scopus 로고
    • D. Coyne, LIGO project (private communication).
    • Coyne, D.1
  • 28
    • 85037906395 scopus 로고    scopus 로고
    • The data for the predicted noise power spectra for the initial and advanced LIGO detectors were taken from, Those for the VIRGO detector were supplied by Luca Gammaitoni (E-mail address: gammaitoni@perugia.infn.it);, the GEO-600 detector by Albrecht Rudiger and Kenneth Strain (E-mail address: atr@mpq.mpg.de and kstrain@physics.gla.ac.uk);, and the TAMA-300 detector by Masa-Katsu Fujimoto (E-mail address: fujimoto@gravity.mtk.nao.ac.jp)., The predicted noise power spectra for the “enhanced” LIGO detectors were supplied by Rainer Weiss (E-mail address: weiss@tristan.mit.edu).
    • The data for the predicted noise power spectra for the initial and advanced LIGO detectors were taken from 1.Those for the VIRGO detector were supplied by Luca Gammaitoni (E-mail address: gammaitoni@perugia.infn.it);the GEO-600 detector by Albrecht Rudiger and Kenneth Strain (E-mail address: atr@mpq.mpg.de and kstrain@physics.gla.ac.uk);and the TAMA-300 detector by Masa-Katsu Fujimoto (E-mail address: fujimoto@gravity.mtk.nao.ac.jp).The predicted noise power spectra for the “enhanced” LIGO detectors were supplied by Rainer Weiss (E-mail address: weiss@tristan.mit.edu).
  • 29
    • 85037912836 scopus 로고    scopus 로고
    • B. Allen, “GRASP: a data analysis package for gravitational wave detection,” 1997. An up-to-date version of the users manual may be obtained at http://www.ligo.caltech.edu/LIGO_web/Collaboration/manual.pdf or http://www.ligo.caltech.edu/LIGO_web/Collaboration/lsc_interm.html. The software package is available upon request.
    • B. Allen, “GRASP: a data analysis package for gravitational wave detection,” 1997. An up-to-date version of the users manual may be obtained at http://www.ligo.caltech.edu/LIGO_web/Collaboration/manual.pdf or http://www.ligo.caltech.edu/LIGO_web/Collaboration/lsc_interm.html. The software package is available upon request.
  • 32
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    • J.M. Lees and J. Park, Compu. Geol. 21, 199 (1995). The multitaper spectral estimation public domain package can be found at the website http://love.geology.yale.edu/mtm/.
    • (1995) Compu. Geol. , vol.21 , pp. 199
    • Lees, J.M.1    Park, J.2


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.