Parameter estimation for binary black holes with networks of third-generation gravitational-wave detectors
Parameter estimation for binary black holes with networks of third-generation gravitational-waveaThe two binary black hole (BBH) coalescences detected by LIGO, GW150914, and GW151226, were relatively nearby sources, with a redshift of ∼ 0.1. As the sensitivity of Advanced LIGO and Virgo increases in...
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| Format: | Article |
| Language: | English |
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American Physical Society
2017
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| Online Access: | http://hdl.handle.net/1721.1/109577 https://orcid.org/0000-0003-2700-0767 https://orcid.org/0000-0001-8459-4499 |