Table 5
Summary of the selections ordered by median redshift.
| Selection | Photometry | Magnitude selection | Density | Median | ID rate | Efficiency | Efficiency | √? | |
| name | upper bound | [deg-2] | redshift | 0.6 <z< 1 | 0.7 <z< 1.1 | ||||
|
|
|||||||||
| gri-Uri | 1 | g< 22.5 or U< 22.5 | 197 | 0.734 | 0.68 | 0.52 | 0.40 | x | |
| griW | 2 | g< 22.5 | 196 | 0.767 | 0.72 | 0.56 | 0.42 | x | |
| UgrizW bright all | 3 | g< 22.5 | 196 | 0.778 | 0.78 | 0.59 | 0.49 | x | |
| UgrizW | 3 | g< 22.7 | 199 | 0.788 | 0.76 | 0.59 | 0.52 | x | |
| des bright | 4 | g< 22.8 | 615 | 0.843 | 0.76 | 0.53 | 0.53 | x | |
| des faint | 4 | r< 22.8 | 650 | 0.901 | 0.71 | 0.41 | 0.47 | x | |
|
|
|||||||||
| Fisher griW optimized | 2 | g< 22.5 | 182 | 0.76 | 0.85 | 0.71 | 0.54 | ~√ | |
| decam 180 | 4 | g< 22.8 | 182 | 0.864 | 0.87 | 0.7 | 0.76 | √ | |
Notes. The efficiency is the number density of galaxies identified in the redshift range specified divided by the total number density of galaxies. The column photometry lists the combination of photometry. 1: SCUSS + SDSS, 2: SCUSS + SDSS + WISE, 3: SDSS + WISE, and 4: DECam. The uncertainties on the number densities and efficiencies are comprised between 1.5 and 3 percent, but for the sake of readability, we report all uncertainties in the tables in Appendix A. The last column reports whether the efficiency requirement are met (the density requirement is always met).
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