Noise characterization for laser interferometer gravitational wave detectors

General Relativity and Gravitation

Volumn 32, Issue 3, 2000, Pages 411-423

  Whiting, B F ^a,b   Coldwell, B L ^a   Scott, S M ^a   Evans, B J ^a   McClelland, D E ^a  

^a AUSTRALIAN NATIONAL UNIVERSITY   (Australia)

^b University of Florida   (United States)

Author keywords

Data analysis for gravitational wave detectors

Indexed keywords

EID: 0034348308     PISSN: 00017701     EISSN: None     Source Type: Journal    
DOI: 10.1023/A:1001916031271     Document Type: Article

References (26)

1. 1. Saulson, P. R. (1994). Fundamentals of Interferometric Gravitational Wave Detectors (World Scientific, Singapore).
2. 2. Abramowici, A. et al. (1992). Science 256, 325.
3. 3. Bradschia, C., et al. (1991). In Gravitational Astronomy: Instrument Design and Astrophysical Prospects, D. E. McClelland and H.-A. Bachor, eds. (World Scientific, Singapore), p. 110-135.
4. 4. Tsubono, K., and the TAMA collaboration (1997). In Gravitational Wave Detection: Proc. TAMA Workshop, K. Tsubono, M.-K. Fujimoto and K. Kuroda, eds. (Universal Academic Press, Tokyo), p. 183-191.
5. 5. De Salvo, R. (1997). "Non Stochastic Noise in Gravitational Wave Detectors." VIRGO preprint.
6. 6. Niebauer, T. M., et al. (1991). Phys. Rev. A43, 5022.
7. 7. Meera, B. J., and Strain, K. (1991). Phys. Rev. A44, 4693.
8. 8. Thorne, K. S. (1989). "Light scattering and proposed baffle configuration." Unpublished Caltech report. See also LIGO technical reports T940063-00, T950101 00, T950132-00 and T960012-00 by E. E. Flanagan and K. S. Thorne.
9. 9. Vinet, J.-Y., Brisson, V., and Braccini, S. (1996). Phys. Rev. D54, 1276.
10. 10. Vinet, J.-Y., Brisson, V., Braccini, S., Ferrante, I., Pinard, L., Bondu, F., and Tournie, E. (1997). Phys. Rev. D56, 6085.
11. 11. Beccaria, M., et al. (1998). Nuc. Instr. and Meth. in Phys. Res. A404, 455.
12. 12. Allen, B. (1998). GRASP Users Manual, University of Wisconsin, Milwaukee.
13. 13. Mours, B. (1997). In Gravitational Wave Detection: Proc. TAMA Workshop, K. Tsubono, M.-K. Fujimoto and K. Kuroda, eds. (Universal Academic Press, Tokyo), p. 27-30. See also the LIGO/VIRGO technical note LIGOT970130-B or VIRGO-SPE-LAP-5400-102.
14. 14. Sigg, D., Fritschel, P. (1998). "LIGO Channel Count." LIGO Technical Document T98000-1-00-D.
15. 15. Schutz, B. F. (1991). In The Detection of Gravitational Radiation, D. G. Blair, ed. (Cambridge University Press, Cambridge), p. 406-452.
16. 16. Pizzella, G. (1997). Class. Quantum Grav. 14, 1481.
17. 17. Nicholson, D., et al. (1996). Phys. Lett. A218, 175.
18. 18. Sintes, A. M., and Schutz, B. F. (1998). Phys. Rev. D58, 122003.
19. 19. Allen, B., and Ottewill, A. (2000). Gen. Rel. Grav. 32, 385 in this special issue.
20. 20. Astone, P., Lobo, J. A., and Schutz, B. F. (1994). Class. Quantum Grav. 11, 2093.
21. 21. Lyne, A. G. (1989). In Gravitational Wave Data Analysis, B. F. Schutz, ed. (Kluwer Academic Publishers, Dordrecht), p. 95.
22. 22. Astrom, K. J., Goodwill, G. C., and Kumar, P. R. (1995). Adaptive Control, Filtering, and Signal Processing (Springer-Verlag, New York).
23. 23. Sandeman, R. J., et al. (1997). A.I.G.O. Prospectus (University of Western Autralia, Perth).
24. 24. Hawick, K. A. (1998). AARNet2 Demonstration Project: Advanced & Distributed Computing Project Plan (University of Adelaide, Adelaide).
25. 26. Heng, I. S., et al. (1996). Phys. Lett. A218, 190.
26. 27. Coldwell, R. L., and Bamford, G. J. (1991). The Theory and Operation of Spectral Analysis - Robfit (A.I.P., New York).