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...
| Main Authors: | , , , , , , , , , , , , , , , , , , , , , , , , , |
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| Format: | Article |
| Language: | en_US |
| Published: |
American Physical Society
2014
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| 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 |