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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

Table 1.

Number of Injected Signals for Each Morphology at Different Stages of the Analysis

SG G WNB BBH
Triggers produced by cWB 1112 256 769 2488
Left out to reduce computational costs 0 0 0 −1988

Analyzed by BW 1112 256 769 500
Identified as glitches or Gaussian noise by BW −779 0 −355 −1

Used in our analysis 333 256 414 499

Note. For details on why BW identified many SG and WNB signals as glitches or Gaussian noise, and how this has been improved for O2, see Appendix A.