LISA data analysis: Source identification and subtraction

Neil J. Cornish and Shane L. Larson
Phys. Rev. D 67, 103001 – Published 12 May 2003
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Abstract

The Laser Interferometer Space Antenna will operate as an AM-FM receiver for gravitational waves. For binary systems, the source location, orientation and orbital phase are encoded in the amplitude and frequency modulation. The same modulations spread a monochromatic signal over a range of frequencies, making it difficult to identify individual sources. We present a method for detecting and subtracting individual binary signals from a data stream with many overlapping signals.

  • Received 29 January 2003

DOI:https://doi.org/10.1103/PhysRevD.67.103001

©2003 American Physical Society

Authors & Affiliations

Neil J. Cornish

  • Department of Physics, Montana State University, Bozeman, Montana 59717

Shane L. Larson

  • Space Radiation Laboratory, California Institute of Technology, Pasadena, California 91125

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Issue

Vol. 67, Iss. 10 — 15 May 2003

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