Table 1
Number of galaxies and volumes for the four subsamples analysed in this paper, compared to the “full” survey. Volumes are in units of 106h-3 Mpc3.
| W1 | W4 | |||||||
|
|
||||||||
| z-range | Ngal | V | Veff | zeff | Ngal | V | Veff | zeff |
|
|
||||||||
| 0.6–0.9 | 28 156 | 9.8 | 9.3 | 0.73 | 14 072 | 5.3 | 5.0 | 0.73 |
| 0.9–1.1 | 6580 | 8.8 | 7.4 | 0.98 | 2920 | 4.7 | 4.0 | 0.97 |
|
|
||||||||
| “Full” VIPERS (0.4-1.2) | 48 754 | 27.4 | 23.5 | 0.70 | 24 323 | 14.8 | 12.7 | 0.70 |
Notes. Effective volumes are defined following Tegmark et al. (2006), using a reference galaxy power spectrum amplitude of Peff = 4000 h-3 Mpc3, as obtained at keff = 0.10 h Mpc-1.
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