The Mock LISA Data Challenges: from Challenge 1B to Challenge 3
| dc.creator | Babak, Stanislav | |
| dc.creator | Baker, John G. | |
| dc.creator | Benacquista, Matthew J. | |
| dc.creator | Cornish, Neil J. | |
| dc.creator | Crowder, Jeff | |
| dc.creator | Larson, Shane L. | |
| dc.creator | Plagnol, Eric | |
| dc.creator | Porter, Edward K. | |
| dc.creator | Vallisneri, Michele | |
| dc.creator | Vecchio, Alberto | |
| dc.creator | Arnaud, Keith | |
| dc.creator | Barack, Leor | |
| dc.creator | Błaut, Arkadiusz | |
| dc.creator | Cutler, Curt | |
| dc.creator | Fairhurst, Stephen | |
| dc.creator | Gair, Jonathan | |
| dc.creator | Gong, Xuefei | |
| dc.creator | Harry, Ian | |
| dc.creator | Khurana, Deepak | |
| dc.creator | Królak, Andrzej | |
| dc.creator | Mandel, Ilya | |
| dc.creator | Prix, Reinhard | |
| dc.creator | Sathyaprakash, B. S. | |
| dc.creator | Savov, Pavlin | |
| dc.creator | Shang, Yu | |
| dc.creator | Trias, Miquel | |
| dc.creator | Veitch, John | |
| dc.creator | Wang, Yan | |
| dc.creator | Wen, Linqing | |
| dc.creator | Whelan, John T. | |
| dc.date | 2008-06-12 | |
| dc.date | 2009-04-15 | |
| dc.date.accessioned | 2026-07-07T13:03:33Z | |
| dc.date.available | 2026-07-07T13:03:33Z | |
| dc.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 article we provide a critical analysis of 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 article 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. | |
| dc.description | 20 pages, 3 EPS figures. Proceedings of the 12th Gravitational Wave Data Analysis Workshop, Cambridge MA, 13--16 December 2007. Typos corrected | |
| dc.identifier | https://arxiv.org/abs/0806.2110 | |
| dc.identifier | http://arxiv.org/abs/0806.2110 | |
| dc.identifier | Class.Quant.Grav.25:184026,2008 | |
| dc.identifier | doi:10.1088/0264-9381/25/18/184026 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/226842 | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.title | The Mock LISA Data Challenges: from Challenge 1B to Challenge 3 | |
| dc.type | text |