LIGO observed a clear gravitational-wave chirp from the merger of two black holes with masses 36 and 29 solar masses at 410 Mpc distance, matching general relativity predictions with signal-to-noise ratio 24.
Weiss, Electromagnetically coupled broadband gravi- tational antenna, Quarterly Report of the Research Labo- ratory for Electronics, MIT Report No
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Observation of Gravitational Waves from a Binary Black Hole Merger
LIGO observed a clear gravitational-wave chirp from the merger of two black holes with masses 36 and 29 solar masses at 410 Mpc distance, matching general relativity predictions with signal-to-noise ratio 24.