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. Author manuscript; available in PMC: 2018 Apr 30.
Published in final edited form as: Astrophys J. 2017 Apr 7;839(No 1):15. doi: 10.3847/1538-4357/aa63ef

Figure 6.

Figure 6

Dependence of network overlaps (𝒪net) on network signal-to-noise ratios (S/Nnet) for SG, G, WNB, and BBH signals. Note that we excluded the injections with S/Nnet > 100 from the curve estimation. Shaded areas represent the 1σ uncertainty regions of the measured 𝒪net values. The left panel shows the S/Nnet dependence of 𝒪net for SG, G, and WNB signals. All three morphologies show a clear trend of increasing overlap with increasing S/Nnet. The right panel shows the S/Nnet dependence of network overlaps for BBH signals with a detector-frame total mass below and above the median total mass M̂tot = 44.49 M⊙. BW performed significantly better for signals with higher Mtot at S/Nnet ≲ 35 values.