Table 1
VIPERS subsamples.
| z-range | MB– cut | nVIPERS | nmock |
| MB − 5log (h) | 10-3h3 Mpc-3 | 10-3h3 Mpc-3 | |
|
|
|||
| 0.5−0.7 | −18.6 − z | 4.78 | 4.36 |
| 0.5−0.7 | −19.1 − z | 3.16 | 2.43 |
| 0.5−0.7 | −19.5 − z | 2.10 | 1.37 |
| 0.5−0.7 | −19.9 − z | 1.24 | 0.68 |
|
|
|||
| 0.7−0.9 | −19.1 − z | 2.71 | 2.55 |
| 0.7−0.9 | −19.5 − z | 1.86 | 1.47 |
| 0.7−0.9 | −19.9 − z | 1.07 | 0.72 |
|
|
|||
| 0.9−1.1 | −19.5 − z | 0.62 | 0.63 |
| 0.9−1.1 | −19.9 − z | 0.42 | 0.43 |
|
|
|||
| 0.5−0.7 | −19.7 − z | 1.64 | 1.36 |
| 0.7−0.9 | −19.7 − z | 1.13 | 1.05 |
| 0.9−1.1 | −19.7 − z | 0.53 | 0.53 |
| 0.7−0.9 | −20.0 | 1.42 | 1.49 |
Notes. Column 1: redshift range. Column 2: B-band magnitude cut (computed for h = 1). Column 3: galaxy number density in the real VIPERS sub-catalogues. Column 4: galaxy number density in the HOD-mock VIPERS sub-catalogues. In the Parent mock catalogue the number density is a factor ~3.7 larger. Cells fully contained in the surveyed volume (i.e. not overlapping with gaps or empty areas) contain ~40% more objects on average.
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