Parameter estimation for compact binary coalescence signals with the first generation gravitational-wave detector network

Parameter estimation for compact binary coalescence signals with the first generation gravitational-wave detector network

Compact binary systems with neutron stars or black holes are one of the most promising sources for ground-based gravitational-wave detectors. Gravitational radiation encodes rich information about source physics; thus parameter estimation and model selection are crucial analysis steps for any detect...

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Main Authors: Barsotti, Lisa (Contributor), Bodiya, Timothy Paul (Contributor), Corbitt, Thomas R. (Contributor), Donovan, Frederick J. (Contributor), Dwyer, S. (Contributor), Evans, Matthew J. (Contributor), Foley, S. (Contributor), Fritschel, Peter K. (Contributor), Katsavounidis, Erotokritos (Contributor), Kissel, Jeffrey S. (Contributor), Kwee, Patrick (Contributor), MacInnis, Myron E. (Contributor), Mason, Kenneth R. (Contributor), Matichard, Fabrice (Contributor), Mavalvala, Nergis (Contributor), Mittleman, Richard K. (Contributor), Oelker, Eric Glenn (Contributor), Sankar, S. (Contributor), Shapiro, B. (Contributor), Shoemaker, David H. (Contributor), Smith-Lefebvre, N. D. (Contributor), Vaulin, Ruslan (Contributor), Waldman, S. J. (Contributor), Weiss, Ron (Contributor), Wipf, Christopher (Contributor), Zucker, Michael E. (Contributor)
Other Authors: Massachusetts Institute of Technology. Department of Physics (Contributor), MIT Kavli Institute for Astrophysics and Space Research (Contributor), LIGO (Observatory : Massachusetts Institute of Technology) (Contributor)
Format: Article
Language:English
Published: American Physical Society, 2014-02-10T17:16:41Z.
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