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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 5.

Figure 5

Cumulative distribution function (CDF) of network overlaps (𝒪net). Shadings represent the 2σ uncertainties calculated using the Dvoretzky-Kiefer– Wolfowitz inequality (Dvoretzky et al. 1956). The lower the curves reach at a given 𝒪net value, the better the reconstruction. The inset shows the normalized histogram of the network signal-to-noise ratio (S/Nnet) for signals with four different morphologies. The curves for SG and G signals are identical within the 2σ statistical errors, and they indicate significantly better reconstructions of SG and G signals than of WNB and BBH signals.