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Measuring a binary's orientation with LISA

MPG-Autoren
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Danzmann,  K.
Laser Interferometry & Gravitational Wave Astronomy, AEI-Hannover, MPI for Gravitational Physics, Max Planck Society;

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Schutz,  B. F.
Astrophysical Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society;

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AdSpR_32_1267J.pdf
(Verlagsversion), 271KB

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Zitation

Jennrich, O., Peterseim, M., Danzmann, K., & Schutz, B. F. (2003). Measuring a binary's orientation with LISA. Advances in Space Research, 32(7), 1267-1270. doi:10.1016/S0273-1177(03)90330-9.


Zitierlink: http://hdl.handle.net/11858/00-001M-0000-0013-753D-D
Zusammenfassung
We are presenting numerical results concerning LISA's ability to distinguish between different polarizational states of a gravitational wave. Therefore, we assume a binary as a source of a gravitational wave, finding its orientation which determines the polarization of the gravitational wave. By means of signal processing, we are able to give the 1σ-uncertainty for determining the orientation of the source.