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Properties of the Binary Black Hole Merger GW150914
Phys. Rev. Lett. 116, 241102 – Published 14 June, 2016
DOI: https://doi.org/10.1103/PhysRevLett.116.241102
Abstract
On September 14, 2015, the Laser Interferometer Gravitational-Wave Observatory (LIGO) detected a gravitational-wave transient (GW150914); we characterize the properties of the source and its parameters. The data around the time of the event were analyzed coherently across the LIGO network using a suite of accurate waveform models that describe gravitational waves from a compact binary system in general relativity. GW150914 was produced by a nearly equal mass binary black hole of masses and ; for each parameter we report the median value and the range of the 90% credible interval. The dimensionless spin magnitude of the more massive black hole is bound to be (at 90% probability). The luminosity distance to the source is , corresponding to a redshift assuming standard cosmology. The source location is constrained to an annulus section of , primarily in the southern hemisphere. The binary merges into a black hole of mass and spin . This black hole is significantly more massive than any other inferred from electromagnetic observations in the stellar-mass regime.
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