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          Institute: MPI für Gravitationsphysik     Collection: Observational Relativity and Cosmology     Display Documents



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ID: 379297.0, MPI für Gravitationsphysik / Observational Relativity and Cosmology
The Mock LISA Data Challenges: from Challenge 1B to Challenge 3
Authors:Babak, Stanislav; Baker, John G.; Benacquista, Matthew J.; Cornish, Neil J.; Crowder, Jeff; Larson, Shane L.; Plagnol, Eric; Porter, Edward; Vallisneri, Michele; Vecchio, Alberto; Arnaud, Keith A.; Barack, Leor; Blaut, Arkadiusz; Cutler, Curt; Fairhurst, Stephen; Gair, Jonathan; Gong, Xuefei; Harry, Ian; Khurana, Deepak; Krolak, Andrzej; Mandel, Ilya; Prix, Reinhard; Sathyaprakash, B. S.; Savov, Pavlin; Shang, Yu; Trias, Miquel; Veitch, John; Wang, Yan; Wen, Linqing; Whelan, John T.
Date of Publication (YYYY-MM-DD):2008-09-21
Title of Journal:Classical and Quantum Gravity
Journal Abbrev.:Class. Quantum Gravity
Volume (in Journal):25
Issue / Number:18
Sequence Number:184026
Name of Conference/Meeting:12th Gravitational Wave Data Analysis Workshop
Place of Conference/Meeting:Cambridge, MA
(Start) Date of Conference/Meeting
 (YYYY-MM-DD):
2007-12-13
End Date of Conference/Meeting 
 (YYYY-MM-DD):
2007-12-16
Review Status:not specified
Audience:Not Specified
Abstract / Description: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.
External Publication Status:published
Document Type:Conference-Paper
Communicated by:Bruce Allen
Affiliations:MPI für Gravitationsphysik/Teilinstitut Hannover
MPI für Gravitationsphysik/Observational Relativity and Cosmology
Identifiers:ISI:000258916700027 [ID No:1]
ISSN:0264-9381 [ID No:2]
DOI:10.1088/0264-9381/25/18/184026
LOCALID:arXiv:0806.2110v1 [gr-qc]
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0806.2110v1.pdf  [417,00 Kb] [Comment:arXiv:0806.2110v1 [gr-qc]]  
 
cqg8_18_184026.pdf  [487,00 Kb] [Comment:Online Journal]  
 
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