Open Access
Table B.1.
Fraction of N90 galaxies removed after applying different optical color cuts with LSST filters.
| Color | u − g | g − r | r − i | i − z |
|---|---|---|---|---|
| Hosts lost | 5% | |||
| Color cut | > 1.59 | > 0.80 | < 1.25 | < 0.92 |
| N90 reduction | 19.23% | 4.16% | 19.69% | 27.70% |
| Hosts lost | 10% | |||
| Color cut | > 1.65 | > 0.87 | < 1.25 | < 0.73 |
| N90 reduction | 20.12% | 6.25% | 19.69% | 34.21% |
| Hosts lost | 20% | |||
| Color cut | > 1.66 | > 0.87 | < 0.58 | < 0.33 |
| N90 reduction | 24.80% | 6.25% | 75.00% | 77.14% |
Notes. The host lost refers to the probability that the true host is removed after the color cut. These numbers only consider the galaxies associated with CGWs whose S/N > 25.
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