Neil J Cornish 2002 Class. Quantum Grav. 19 1279 doi:10.1088/0264-9381/19/7/306
Neil J Cornish
Show affiliationsThe laser interferometer space antenna (LISA) can be used to map the gravitational wave background by measuring the orbital modulation of the detector response. Using the known antenna pattern and orbit, and the measured modulation, it is possible to solve for the sky luminosity distribution.
Issue 7 (7 April 2002)
Received 29 October 2001, in final form 29 November 2001
Published 11 March 2002
Neil J Cornish 2002 Class. Quantum Grav. 19 1279
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