Table A.1
Incompleteness and contamination of the VIPERS galaxy sample expected from the star–galaxy separation process, estimated by applying the final criteria discussed in the text to the VVDS Deep and Wide complete catalogues to iAB = 22.5.
| Field | Inc | Cnt |
| W1 (VVDS-Deep) | 2.07% (2.13)% | 0.87% (0.27%) |
| W4 (VVDS-Wide) | 0.96% (0.64%) | 6.59% (8.24%) |
Notes. The values in parentheses give the values corresponding to galaxies colour-selected to be at z> 0.5, i.e. that would be part of the actual VIPERS target (Sect. 4).
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