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  Position determination of gravitational wave sources with LISA

Jennrich, O., Peterseim, M., Danzmann, K., & Schutz, B. F. (2003). Position determination of gravitational wave sources with LISA. Advances in Space Research, 32(7), 1263-1266. doi:10.1016/S0273-1177(03)90329-2.

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Item Permalink: http://hdl.handle.net/11858/00-001M-0000-0013-1193-7 Version Permalink: http://hdl.handle.net/11858/00-001M-0000-0013-1196-1
Genre: Journal Article

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AdSpR_32_1263.pdf (Publisher version), 334KB
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 Creators:
Jennrich, O.1, Author
Peterseim, M.1, Author
Danzmann, K.2, Author              
Schutz, B. F.3, Author              
Affiliations:
1External Organizations, ou_persistent22              
2Laser Interferometry & Gravitational Wave Astronomy, AEI-Hannover, MPI for Gravitational Physics, Max Planck Society, Hannover, DE, ou_24010              
3Astrophysical Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society, Golm, DE, ou_24013              

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 Abstract: 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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 Dates: 2003-10
 Publication Status: Published online
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 Rev. Method: Peer
 Identifiers: DOI: 10.1016/S0273-1177(03)90329-2
eDoc: 335757
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Title: Advances in Space Research
Source Genre: Journal
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Pages: - Volume / Issue: 32 (7) Sequence Number: - Start / End Page: 1263 - 1266 Identifier: ISSN: 0273-1177