Gravitational-wave localization alone can probe origin of stellar-mass black hole mergers.

Nat Commun · 2017 · PMC5635124 · PMID 29018247

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marginally significantno p-value reported

With higher host number densities it becomes difficult to prove an AGN connection solely using GW localizations, although the construction of additional GW detectors (Kamioka Gravitational Wave Detector, or KAGRA 26 and LIGO India 4 ), and potentially the inclusion of marginally significant GW events, will further improve the situation.

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