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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 1.

Figure 1

Normalized histograms of angular offsets (δθ) for injections with four different morphologies (SG, G, WNB, and BBH). Most of the injected signals have cos(δθ) = 1, which indicates that BW tends to place the most probable location close to the true location. Note that the distributions for different morphologies are very similar to each other, which means that the angular offset does not depend strongly on signal morphology. The complete figure set (three figures) showing the same plot for cWB and LIB pipelines is available in the online journal.

(The complete figure set (3 images) is available.)