Discriminating a gravitational wave background from instrumental noise in the LISA detector

Physical Review D

Volumn 63, Issue 2, 2001, Pages

  Tinto, Massimo ^a   Armstrong, J W ^a   Estabrook, F B ^a  

^a CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

ARTICLE; COSMOS; GRAVITY; INTERFEROMETER; LASER; MATHEMATICAL ANALYSIS; NOISE; PHASE TRANSITION;

EID: 0035862255     PISSN: 05562821     EISSN: None     Source Type: Journal    
DOI: 10.1103/PhysRevD.63.021101     Document Type: Article

References (8)

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3. D. Hils, P. L. Bender and R. F. Webbink, Astrophys. J. 360, 75 (1990).
4. R. F. Webbink, Astrophys. J. 277, 355 (1984).
5. M. Tinto and J. W. Armstrong, Phys. Rev. D 59, 102003 (1999).
6. J. W. Armstrong, F. B. Estabrook, and M. Tinto, Astrophys. J. 527, 814 (1999).
7. F. B. Estabrook, M. Tinto, and J. W. Armstrong, Phys. Rev. D 62, 042002 (2000).
8. P. Bender, K. Danzmann, and the LISA Study Team, Laser Interferometer Space Antenna for the Detection of Gravitational Waves, Pre-Phase A Report, MPQ233 (Max-Planck-Institüt für Quantenoptik, Garching, 1998).