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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Bibliographic Details
Main Authors: Barsotti, Lisa, Bodiya, Timothy Paul, Corbitt, Thomas R., Donovan, Frederick J., Dwyer, S., Evans, Matthew J., Foley, S., Fritschel, Peter K., Katsavounidis, Erotokritos, Kissel, Jeffrey S., Kwee, Patrick, MacInnis, Myron E., Mason, Kenneth R., Matichard, Fabrice, Mavalvala, Nergis, Mittleman, Richard K., Oelker, Eric Glenn, Sankar, S., Shapiro, B., Shoemaker, David H., Smith-Lefebvre, N. D., Vaulin, Ruslan, Waldman, S. J., Weiss, Ron, Wipf, Christopher, Zucker, Michael E.
Other Authors: Massachusetts Institute of Technology. Department of Physics
Format: Article
Language:en_US
Published: American Physical Society 2014
Online Access:http://hdl.handle.net/1721.1/84921
https://orcid.org/0000-0003-0396-2443
https://orcid.org/0000-0003-0219-9706
https://orcid.org/0000-0003-2815-7387
https://orcid.org/0000-0001-6550-3045
https://orcid.org/0000-0002-4147-2560
https://orcid.org/0000-0001-8459-4499
https://orcid.org/0000-0002-2544-1596
https://orcid.org/0000-0003-1983-3187

Internet

http://hdl.handle.net/1721.1/84921
https://orcid.org/0000-0003-0396-2443
https://orcid.org/0000-0003-0219-9706
https://orcid.org/0000-0003-2815-7387
https://orcid.org/0000-0001-6550-3045
https://orcid.org/0000-0002-4147-2560
https://orcid.org/0000-0001-8459-4499
https://orcid.org/0000-0002-2544-1596
https://orcid.org/0000-0003-1983-3187

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