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# GW170608: Observation of a 19 solar-mass binary black hole coalescence

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## Abstract

On 2017 June 8 at 02:01:16.49 UTC, a gravitational-wave (GW) signal from the merger of two stellar-mass black holes was observed by the two Advanced Laser Interferometer Gravitational-Wave Observatory detectors with a network signal-to-noise ratio of 13. This system is the lightest black hole binary so far observed, with component masses of ${12}_{-2}^{+7}\,{M}_{\odot }$ and ${7}_{-2}^{+2}\,{M}_{\odot }$ (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 GWs with electromagnetic observations. The source's luminosity distance is ${340}_{-140}^{+140}\,\mathrm{Mpc}$, corresponding to redshift ${0.07}_{-0.03}^{+0.03}$. We verify that the signal waveform is consistent with the predictions of general relativity.

Item Type: Article Publication Published Advanced Research Computing @ Cardiff (ARCCA)Physics and Astronomy Q Science > QB AstronomyQ Science > QC Physics LIGO Scientific Collaboration and Virgo Collaboration. Original content from this work may be used under the termsof the Creative Commons Attribution 3.0 licence. American Astronomical Society 2041-8205 8 January 2018 2 December 2017 24 Feb 2021 13:51 http://orca.cf.ac.uk/id/eprint/107988

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