Table 1.
Summary of the spectroscopic data used in this work.
| Data | # objects in KiDS | # unique objects | z16% | z50% | z84% | mr, 16% | mr, 50% | mr, 84% |
|---|---|---|---|---|---|---|---|---|
| GAMA | 233 046 | 233 046 | 0.12 | 0.22 | 0.34 | 18.7 | 19.6 | 20.1 |
| SDSS | 99 253 | 77 371 | 0.09 | 0.37 | 0.57 | 17.7 | 19.7 | 21.1 |
| 2dFLenS | 37 462 | 34 253 | 0.13 | 0.30 | 0.59 | 18.3 | 19.5 | 21.0 |
| COSMOS (GAMA-G10) | 20 324 | 20 324 | 0.32 | 0.68 | 1.24 | 21.6 | 22.9 | 24.0 |
Notes. The first three columns are the spectroscopic data sets under consideration, their total number of objects in KiDS DR4, and the unique number of objects in each data set. The next three columns are the 16th, 50th, and 84th percentiles of the spectroscopic redshifts of the unique objects in the spectroscopic data sets. The last three columns are the 16th, 50th, and 84th percentiles of the KiDS GAaP r-band magnitudes of the objects in each spec-z data. For each row, the unique number of objects is obtained after removing the objects that are already included in the GAMA catalogue (GAMA or SDSS catalogues) in the case of SDSS (2dFLenS).
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