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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Bibliographic Details
Main Authors: Vitale, Salvatore (Contributor), Evans, Matthew J (Contributor)
Other Authors: Massachusetts Institute of Technology. Department of Physics (Contributor), MIT Kavli Institute for Astrophysics and Space Research (Contributor)
Format: Article
Language:English
Published: American Physical Society, 2017-06-02T23:13:17Z.
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