Scott E Pollack 2004 Class. Quantum Grav. 21 3419 doi:10.1088/0264-9381/21/14/007
Scott E Pollack
Show affiliationsEach spacecraft in the Laser Interferometer Space Antenna (LISA) houses a proof mass which follows a geodesic through spacetime. Disturbances which change the proof mass position, momentum and/or acceleration will appear in the LISA data stream as additive quadratic functions. These data disturbances inhibit signal extraction and must be removed. In this paper we discuss the identification and fitting of monochromatic signals in the data set in the presence of data disturbances. We also present a preliminary analysis of the extent of science result limitations with respect to the frequency of data disturbances.
Issue 14 (21 July 2004)
Received 4 March 2004
Published 21 June 2004
Scott E Pollack 2004 Class. Quantum Grav. 21 3419
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