LISA data analysis: Source identification and subtraction
arXiv:astro-ph/0301548 · doi:10.1103/PhysRevD.67.103001
Abstract
The Laser Interferometer Space Antenna (LISA) 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.
15 pages, 17 figures