AbstractLISA 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.
Position determination of gravitational wave sources with LISA
Advances in Space Research ; 32 , 7 ; 1263-1266
2003-01-01
4 pages
Aufsatz (Zeitschrift)
Elektronische Ressource
Englisch
Position determination of gravitational wave sources with LISA
Online Contents | 2003
|Position Determination of Gravitational Wave Sources with LISA
British Library Conference Proceedings | 2003
|Pioneering gravitational wave astronomy with LISA
British Library Conference Proceedings | 2005
|Optical Metrology Subsystem of the LISA Gravitational Wave Detector
British Library Conference Proceedings | 2006
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