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Volumn 57, Issue 12, 1998, Pages 7089-7102

Angular resolution of the LISA gravitational wave detector

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Indexed keywords


EID: 0000857708     PISSN: 15507998     EISSN: 15502368     Source Type: Journal    
DOI: 10.1103/PhysRevD.57.7089     Document Type: Article
Times cited : (628)

References (24)
  • 4
    • 85037248309 scopus 로고    scopus 로고
    • K. Danzmann et al., LISA Pre-Phase A Report, Max-Planck-Institut fur Quantenoptik, Report No. MPQ 208, Garching, Germany, 1996
    • K. Danzmann et al., LISA Pre-Phase A Report, Max-Planck-Institut fur Quantenoptik, Report No. MPQ 208, Garching, Germany, 1996.
  • 15
    • 85037202915 scopus 로고    scopus 로고
    • J. E. Faller, P. L. Bender, J. L. Hall, and M. A. Vincent, Proceedings of the Colloquium “Kilometric Optical Arrays in Space,” Cargese, France, 1984;, ESA Report No. SP-226, 1985
    • J. E. Faller, P. L. Bender, J. L. Hall, and M. A. Vincent, Proceedings of the Colloquium “Kilometric Optical Arrays in Space,” Cargese, France, 1984;ESA Report No. SP-226, 1985.
  • 16
    • 0003811646 scopus 로고
    • S. W. Hawking, W. Israel, Cambridge University Press, Cambridge, England
    • K. S. Thorne, in 300 Years of Gravitation, edited by S. W. Hawking and W. Israel (Cambridge University Press, Cambridge, England, 1987), pp. 330–458.
    • (1987) 300 Years of Gravitation , pp. 330-458
    • Thorne, K.S.1
  • 19
    • 85037178578 scopus 로고    scopus 로고
    • P. L. Bender and D. Hils (private communication). We note that our definition of the noise spectral density follows the convention of 16.
    • Bender, P.L.1    Hils, D.2


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.