Detection of gravitational waves from inspiraling, compact binaries using a network of interferometric detectors

International Journal of Modern Physics D

Volumn 9, Issue 3, 2000, Pages 325-329

  Bose, Sukanta ^c   Pai, Archana ^a   Dhurandhar, Sanjeev ^a,b  

^a INTER UNIVERSITY CENTRE FOR ASTRONOMY AND ASTROPHYSICS   (India)

^b ALBERT EINSTEIN INSTITUT   (Germany)

^c NONE

Author keywords

[No Author keywords available]

Indexed keywords

EID: 0039591399     PISSN: 02182718     EISSN: None     Source Type: Journal    
DOI: 10.1142/S0218271800000360     Document Type: Article

References (7)

1. See, e.g., K. S. Thorne, in 300 Years of Gravitation, eds. S. Hawking and W. Israel (Cambridge University Press, Cambridge, 1987), and references therein.
2. B. F. Schutz, in The detection of gravitational waves, ed. D. G. Blair (Cambridge University Press, Cambridge, 1992), pp. 406-452.
3. S. Bose, S. V. Dhurandhar, and A. Pai, Pramana 53 (1999) 1125. (gr-qc/9906064)
4. C. W. Helstrom, Statistical Theory of Signal Detection (Pergamon, London, 1968).
5. In defining the Euler angles, we follow the convention of H. Goldstein, Classical Mechanics (Addison-Wesley Publishing Co., Reading, 1980), 2nd ed.
6. I.
7. Rare instances of non-Gaussian noise can be vetoed by techniques similar to those applied for a single detector; see, e.g., B. Allen et al., Phys. Rev. Lett. 83, (1999) 1498.