χ2 testing of optimal filters for gravitational wave signals: An experimental implementation

Physical Review D - Particles, Fields, Gravitation and Cosmology

Volumn 61, Issue 10, 2000, Pages 1-9

  Baggio, L ^a   Cerdonio, M ^a   Ortolan, A ^a   Vedovato, G ^a   Taffarello, L ^a   Zendri, J P ^a   Bonaldi, M ^b   Falferi, P ^b   Martinucci, V ^c   Mezzena, R ^c   Prodi, G A ^c   Vitale, S ^c  

^a SEZIONE DI PADOVA   (Italy)

^b CNR   (Italy)

^c UNIVERSITY OF TRENTO   (Italy)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 17144371493     PISSN: 05562821     EISSN: None     Source Type: Journal    
DOI: 10.1103/PhysRevD.61.102001     Document Type: Article

References (14)

1. S. Vitale et al., Nucl. Phys. B48, 104 (1996).
2. G. A. Prodi et al., in Gravitational Waves: Proceedings of the Second Edoardo Amaldi Conference, CERN, Geneva, 1997, edited by E. Coccia, G. Veneziano, and G. Pizzella (World Scientific, Singapore, 1998), pp. 148-158.
3. C. W. Helstrom, Statistical Theory of Signal Detection (Pergamon, Oxford, 1968).
4. S. Vitale, G. A. Prodi, J. P. Zendri, A. Ortolan, L. Taffarello, G. Vedovato, M. Cerdonio, and D. Pascoli, in Gravitational Waves, Sources and Detectors, Proceedings of the International Conference, edited by F. Fidecaro and I. Ciufolini (World Scientific, Singapore, 1997), p. 256.
5. See, e.g., J. C. Price, Phys. Rev. D 36, 3555 (1987); M. Cerdonio et al., Physica B 194-196, 3 (1994).
6. See, e.g., J. C. Price, Phys. Rev. D 36, 3555 (1987); M. Cerdonio et al., Physica B 194-196, 3 (1994).
7. A. Ortolan, G. Vedovato, M. Cerdonio, and S. Vitale, Phys. Rev. D 50, 4737 (1994).
8. A. Ortolan et al., in Gravitational Waves: Proceedings of the Second Edoardo Amaldi Conference, CERN, Geneva, 1997, edited by E. Coccia, G. Veneziano, and G. Pizzella (Ref. [2]), pp. 204-215.
9. V. Crivelli-Visconti et al., Phys. Rev. D 57, 2045 (1998).
10. L. Baggio et al., Proceedings of the Third Edoardo Amaldi Conference, Caltech, Pasadena, CA, 1999 (in press); G. A. Prodi et al., ibid.
11. L. Baggio et al., Proceedings of the Third Edoardo Amaldi Conference, Caltech, Pasadena, CA, 1999 (in press); G. A. Prodi et al., ibid.
12. Here a purely polarized wave is assumed in order not to make the algebra too heavy. Extension to arbitrary polarization is straightforward.
13. ALLEGRO at University of Louisiana, Baton Rouge, USA, AURIGA at INFN Natl. Lab. of Legnaro, Italy, EXPLORER at CERN, Switzerland, NAUTILUS at INFN Natl. Lab. of Frascati, Italy, and NIOBE at University of Western Australia, Perth, Australia.
14. Within the International Gravitational Event Collaboration, IGEC.