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  The Mock LISA Data Challenges: from Challenge 3 to Challenge 4

Babak, S., Baker, J. G., Benacquista, M. J., Cornish, N. J., Larson, S. L., Mandel, I., et al. (2010). The Mock LISA Data Challenges: from Challenge 3 to Challenge 4. Classical and quantum gravity, 27(8): 084009. doi:10.1088/0264-9381/27/8/084009.

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Item Permalink: http://hdl.handle.net/11858/00-001M-0000-0012-BBC9-E Version Permalink: http://hdl.handle.net/11858/00-001M-0000-0012-BBCB-A
Genre: Journal Article

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 Creators:
Babak, Stanislav1, Author              
Baker, John G., Author
Benacquista, Matthew J., Author
Cornish, Neil J., Author
Larson, Shane L., Author
Mandel, Ilya, Author
McWilliams, Sean T., Author
Petiteau, Antoine1, Author
Porter, Edward K., Author
Robinson, Emma L.1, Author              
Vallisneri, Michele, Author
Vecchio, Alberto, Author
Adams, Matt, Author
Arnaud, Keith A., Author
Błaut, Arkadiusz2, Author
Bridges, Michael, Author
Cohen, Michael2, Author
Cutler, Curt, Author
Feroz, Farhan, Author
Gair, Jonathan R., Author
Graff, Philip, AuthorHobson, Mike, AuthorKey, Joey Shapiro, AuthorKrolak, Andrzej3, Author              Lasenby, Anthony, AuthorPrix, Reinhard3, Author              Shang, Yu1, AuthorTrias, Miquel, AuthorVeitch, John, AuthorWhelan, John T.1, Author               more..
Affiliations:
1Astrophysical Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society, ou_24013              
2the MLDC 3 participants, ou_persistent22              
3Observational Relativity and Cosmology, AEI-Hannover, MPI for Gravitational Physics, Max Planck Society, ou_24011              

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Free keywords: General Relativity and Quantum Cosmology, gr-qc
 Abstract: The Mock LISA Data Challenges are a program to demonstrate LISA data-analysis capabilities and to encourage their development. Each round of challenges consists of one or more datasets containing simulated instrument noise and gravitational waves from sources of undisclosed parameters. Participants analyze the datasets and report best-fit solutions for the source parameters. Here we present the results of the third challenge, issued in Apr 2008, which demonstrated the positive recovery of signals from chirping Galactic binaries, from spinning supermassive--black-hole binaries (with optimal SNRs between ~ 10 and 2000), from simultaneous extreme-mass-ratio inspirals (SNRs of 10-50), from cosmic-string-cusp bursts (SNRs of 10-100), and from a relatively loud isotropic background with Omega_gw(f) ~ 10^-11, slightly below the LISA instrument noise.

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 Dates: 2009-12-022010-01-262010
 Publication Status: Published in print
 Pages: 12 pages, 2 figures, proceedings of the 8th Edoardo Amaldi Conference on Gravitational Waves, New York, June 21-26, 2009
 Publishing info: -
 Table of Contents: -
 Rev. Method: -
 Identifiers: arXiv: 0912.0548
DOI: 10.1088/0264-9381/27/8/084009
URI: http://arxiv.org/abs/0912.0548
 Degree: -

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Title: Classical and quantum gravity
Source Genre: Journal
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Publ. Info: Bristol, U.K. : Institute of Physics
Pages: - Volume / Issue: 27 (8) Sequence Number: 084009 Start / End Page: - Identifier: Other: 954925513480
Other: 0264-9381