Table 1.
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.