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We show that gravitational-wave signals from compact binary mergers may bebetter distinguished from instrumental noise transients by using Bayesianmodels that look for signal coherence across a detector network. This can beachieved even when the signal power is below the usual threshold for detection.This method could reject the vast majority of noise transients, and thereforeincrease sensitivity to weak gravitational waves. We demonstrate this usingsimulated signals, as well as data for GW150914 and LVT151012. Finally, weexplore ways of incorporating our method into existing Advanced LIGO and Virgosearches to make them significantly more powerful.

Enhancing confidence in the detection of gravitational waves from compact binaries using signal coherence