GW170608: Observation of a 19 solar-mass binary black hole coalescence
High Energy Astrophysical Phenomena, General Relativity and Quantum Cosmology
On June 8, 2017 at 02:01:16.49 UTC, a gravitational-wave signal from the merger of two stellar-mass black holes was observed by the two Advanced LIGO detectors with a network signal-to-noise ratio of 13. This system is the lightest black hole binary so far observed, with component masses 12+7−2M⊙ and 7+2−2M⊙ (90% credible intervals). These lie in the range of measured black hole masses in low-mass X-ray binaries, thus allowing us to compare black holes detected through gravitational waves with electromagnetic observations. The source's luminosity distance is 340+140−140 Mpc, corresponding to redshift 0.07+0.03−0.03. We verify that the signal waveform is consistent with the predictions of general relativity.
Astrophysical Journal of Letters
Summerscales, Tiffany; LIGO Scientific Collaboration; and Virgo Collaboration, "GW170608: Observation of a 19 solar-mass binary black hole coalescence" (2017). Faculty Publications. 711.