On August 14, 2017 at 10 30:43 UTC, the Advanced Virgo detector and the two Advanced LIGO detectors coherently observed a transient gravitational-wave signal produced by the coalescence of two stellar mass black holes, with a false-alarm rate of ≲1 in 27 000 years. The signal was observed with a three-detector network matched-filter signal-to-noise ratio of 18. The inferred masses of the initial black holes are 30.5-3.0+5.7M⊙ and 25.3-4.2+2.8M⊙ (at the 90% credible level). The luminosity distance of the source is 540-210+130 Mpc, corresponding to a redshift of z=0.11-0.04+0.03. A network of three detectors improves the sky localization of the source, reducing the area of the 90% credible region from 1160 deg2 using only the two LIGO detectors to 60 deg2 using all three detectors. For the first time, we can test the nature of gravitational-wave polarizations from the antenna response of the LIGO-Virgo network, thus enabling a new class of phenomenological tests of gravity.
B. P. Abbott et al., "GW170814: A Three-Detector Observation of Gravitational Waves from a Binary Black Hole Coalescence," Physical Review Letters, vol. 119, no. 14, American Physical Society (APS), Oct 2017.
The definitive version is available at https://doi.org/10.1103/PhysRevLett.119.141101
Keywords and Phrases
Gravitational effects; Gravity waves; Matched filters; Signal processing; Signal to noise ratio; Stars; Antenna response; Credible regions; Detector networks; False alarm rate; Filter signals; Gravitational-wave signals; Stellar-mass black holes; VIRGO detector; Gravitation
International Standard Serial Number (ISSN)
Article - Journal
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