LIGO Document G1600269-v2
- On September 14, 2015, the Laser Interferometer Gravitational-wave Observatory (LIGO) detected a gravitational-wave transient (GW150914). In this talk I present the inferred properties of the source, showing that it corresponds to a nearly equal mass binary black binary that merges to form a final black hole of approximately 62 solar masses.
- held on 04 Apr 2016 in University of Nottingham
- held from 04 Apr 2016 to 05 Apr 2016 in University of Nottingham
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