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  The Mock LISA Data Challenges: from Challenge 1B to Challenge 3

Babak, S., Baker, J. G., Benacquista, M. J., Cornish, N. J., Crowder, J., Larson, S. L., et al. (2008). The Mock LISA Data Challenges: from Challenge 1B to Challenge 3. Classical and Quantum Gravity, 25(18): 184026. doi:10.1088/0264-9381/25/18/184026.

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 Creators:
Babak, Stanislav1, Author           
Baker, John G.2, Author
Benacquista, Matthew J.2, Author
Cornish, Neil J.2, Author
Crowder, Jeff2, Author
Larson, Shane L.2, Author
Plagnol, Eric2, Author
Porter, Edward K.1, Author
Vallisneri, Michele2, Author
Vecchio, Alberto2, Author
Arnaud, Keith3, Author
Barack, Leor3, Author
Błaut, Arkadiusz3, Author
Cutler, Curt3, Author
Fairhurst, Stephen3, Author
Gair, Jonathan1, Author
Gong, Xuefei3, Author
Harry, Ian3, Author
Khurana, Deepak3, Author
Królak, Andrzej3, Author
Mandel, Ilya3, AuthorPrix, Reinhard4, Author           Sathyaprakash, B. S.3, AuthorSavov, Pavlin3, AuthorShang, Yu3, AuthorTrias, Miquel3, AuthorVeitch, John3, AuthorWang, Yan3, AuthorWen, Linqing1, AuthorWhelan, John T.1, Author            more..
Affiliations:
1Astrophysical Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society, Golm, DE, ou_24013              
2External Organizations, the Mock LISA Data Challenge Task Force, ou_persistent22              
3External Organizations, the Challenge 1B participants, ou_persistent22              
4Observational Relativity and Cosmology, AEI-Hannover, MPI for Gravitational Physics, Max Planck Society, Hannover, DE, ou_24011              

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Free keywords: gr-qc
 Abstract: The Mock LISA Data Challenges are a programme to demonstrate and encourage the development of LISA data-analysis capabilities, tools and techniques. At the time of this workshop, three rounds of challenges had been completed, and the next was about to start. In this paper we provide a critical analysis of the entries to the latest completed round, Challenge 1B. The entries confirm the consolidation of a range of data-analysis techniques for galactic and massive-black-hole binaries, and they include the first convincing examples of detection and parameter estimation of extreme-mass-ratio inspiral sources. In this paper we also introduce the next round, Challenge 3. Its data sets feature more realistic waveform models (e. g., galactic binaries may now chirp, and massive-black-hole binaries may precess due to spin interactions), as well as new source classes (bursts from cosmic strings, isotropic stochastic backgrounds) and more complicated nonsymmetric instrument noise.

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 Dates: 2008-09-21
 Publication Status: Published online
 Pages: -
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 Table of Contents: -
 Rev. Type: Peer
 Identifiers: DOI: 10.1088/0264-9381/25/18/184026
eDoc: 379297
arXiv: 0806.2110
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Title: 12th Gravitational Wave Data Analysis Workshop
Place of Event: Cambridge, MA
Start-/End Date: 2007-12-13 - 2007-12-16

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Title: Classical and Quantum Gravity
Source Genre: Journal
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Pages: - Volume / Issue: 25 (18) Sequence Number: 184026 Start / End Page: - Identifier: ISSN: 0264-9381