LISA data analysis: Source identification and subtraction

Physical Review D - Particles, Fields, Gravitation and Cosmology

Volumn 67, 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

EID: 84865005121     PISSN: 15507998     EISSN: 15502368     Source Type: Journal    
DOI: 10.1103/PhysRevD.67.103001     Document Type: Article

References (22)

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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. (Formula presented) 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.