Position determination of gravitational wave sources with LISA

Details Position determination of gravitational wave sources with LISA Position determination of gravitational wave sources with LISA

Oct 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003adspr..32.1263p&link_type=abstract

Advances in Space Research, Volume 32, Issue 7, p. 1263-1266.

Physics

Scientific paper

LISA is a spaceborne laser interferometer for the detection and observation of gravitational waves, currently under study by ESA. A brief introduction of the main features of this detector, concentrating on its one-year orbital motion around the Sun is given. The amplitude as well as the phase of a gravitational wave is modulated due to that motion, allowing us to extract information from the signal. The detection of monochromatic gravitational waves based on the well-known signal detection theory is simulated, focusing on estimating the angular parameters of the source. The results of the semi-analytic calculations give the angular resolution of LISA.

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