LISA data analysis: Source identification and subtraction

Physical Review D

Volumn 68, Issue 10, 2003, Pages

  Cornish, Neil J ^a   Larson, Shane L ^b  

^a MONTANA STATE UNIVERSITY   (United States)

^b CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

AMPLITUDE MODULATION; ANTENNA; ARTICLE; DATA ANALYSIS; FREQUENCY MODULATION; GRAVITY; INTERFEROMETRY; LASER; LASER INTERFEROMETER SPACE ANTENNA; SIGNAL DETECTION; TECHNIQUE; WAVEFORM;

EID: 33750366624     PISSN: 05562821     EISSN: None     Source Type: Journal    
DOI: 10.1103/PhysRevD.68.103001     Document Type: Article

References (22)

1. P.L. Bender and D. Hils, Class. Quantum Grav. 14, 1439 (1997).
2. D. Hils, P. Bender, and R.F. Webbink, Astrophys. J. 360, 75 (1990).
3. P. Bender et al., LISA Pre-Phase A Report, 2nd ed. (1998).
4. C.J. Hogan and P.L. Bender, Phys. Rev. D 64, 062002 (2001).
5. N.J. Cornish and S. Larson, gr-qc/0206017.
6. S.A. Hughes, Phys. Rev. D 64, 064004 (2001).
7. K. Glampedakis, S.A. Hughes, and D. Kennefick, Phys. Rev. D 66, 064005 (2002).
8. C. Cutler, Phys. Rev. D 57, 7089 (1998).
9. T. Moore and R.W. Hellings, Phys. Rev. D 65, 062001 (2002).
10. R.T. Stebbins, D. Hils, B.K. Bender, and P.L. Bender, talk given at the Third International LISA Symposium, 2000.
11. J. Högbom, Astrophys. J., Suppl. 15, 417 (1974).
12. N.J. Cornish and L.J. Rubbo, Phys. Rev. D 67, 022001 (2003).
13. N.J. Cornish and S. Larson, Class. Quantum Grav. 18, 3473 (2001).
14. P.C. Peters and J. Mathews, Phys. Rev. 131, 435 (1963).
15. C. Hellier, Cataclysmic Variable Stars (Springer-Praxis, London, 2001).
16. National Space Science Data Center, http://nssdc.gsfc.nasa.gov/
17. B. Owen, Phys. Rev. D 53, 6749 (1996).
18. K.M. Gorski, B.D. Wandelt, E. Hivon, F.K. Hansen, and A.J. Banday, astro-ph/9905275; http://www.eso.org/science/healpix/
19. S. Phinney, talk given at the Fourth International LISA Symposium, 2002.
20. Electromagnetic astronomers call the product of this step the CLEAN map.
21. s(f) is the power spectral density due to gravitational waves folded together with the instrumental response function.
22. For example, in Cutler's original treatment of the detector modulation (Ref. [8]), he decomposed the LISA data channels into two overlapping interferometric signals labeled I and II.