O Jennrich et al 1997 Class. Quantum Grav. 14 1525 doi:10.1088/0264-9381/14/6/022
O Jennrich
, M Peterseim
, K Danzmann
,
and B F Schutz
We discuss LISA's ability to resolve different polarizational states of a gravitational wave with fixed frequency and amplitude. Assuming a binary as the source of the gravitational wave, its orientation is connected with the polarization of the gravitational wave emitted. Using methods of signal processing, we calculate the 1-
uncertainty range for measuring the orientation of the source.
04.30.Db Wave generation and sources
97.80.-d Binary and multiple stars
Issue 6 (June 1997)
Received 13 August 1996, in final form 13 January 1997
O Jennrich et al 1997 Class. Quantum Grav. 14 1525
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