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Report on the second Mock LISA Data Challenge

MPG-Autoren
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Babak,  Stanislav
Astrophysical Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society;

Porter,  Edward K.
the Mock LISA Data Challenge task force;
AEI-Golm, MPI for Gravitational Physics, Max Planck Society;

/persons/resource/persons42125

Messenger,  Christopher
Observational Relativity and Cosmology, AEI-Hannover, MPI for Gravitational Physics, Max Planck Society;

/persons/resource/persons20664

Petiteau,  Antoine
Astrophysical Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society;

Pitkin,  Matthew
Laser Interferometry & Gravitational Wave Astronomy, AEI-Hannover, MPI for Gravitational Physics, Max Planck Society;

/persons/resource/persons40534

Prix,  Reinhard
Observational Relativity and Cosmology, AEI-Hannover, MPI for Gravitational Physics, Max Planck Society;
the Challenge 2 participants;

/persons/resource/persons20671

Robinson,  Emma L.
Astrophysical Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society;
the Challenge 2 participants;

/persons/resource/persons1454

Röver,  Christian
Observational Relativity and Cosmology, AEI-Hannover, MPI for Gravitational Physics, Max Planck Society;
the Challenge 2 participants;

Wen,  Linqing
AEI-Golm, MPI for Gravitational Physics, Max Planck Society;
the Challenge 2 participants;

/persons/resource/persons4293

Whelan,  John T.
Astrophysical Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society;
the Challenge 2 participants;

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Zitation

Babak, S., Baker, J. G., Benacquista, M. J., Cornish, N. J., Crowder, J., Cutler, C., et al. (2008). Report on the second Mock LISA Data Challenge. Classical and Quantum Gravity, 25(11): 114037. doi:10.1088/0264-9381/25/11/114037.


Zitierlink: https://hdl.handle.net/11858/00-001M-0000-0013-6215-2
Zusammenfassung
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 several data sets containing simulated instrument noise and gravitational-wave sources of undisclosed parameters. Participants are asked to analyze the data sets and report the maximum information about source parameters. The challenges are being released in rounds of increasing complexity and realism: in this proceeding we present the results of Challenge 2, issued in January 2007, which successfully demonstrated the recovery of signals from supermassive black-hole binaries, from ~20,000 overlapping Galactic white-dwarf binaries, and from the extreme-mass-ratio inspirals of compact objects into central galactic black holes.