Table 3
Best-fit parameters obtained for the real-space correlation function ξ(r) of the original sample and the recovered deprojected correlation function ξdep(r) for the mock photometric redshift samples.
Redshift uncertainty  |
r0 (h-1 Mpc) |
γ |
|
|
||
| z c | 13.16 ± 0.17 | 2.0 (fixed) |
| 13.20 ± 0.23 | 1.97 ± 0.05 | |
|
|
||
| 0.001 | 12.82 ± 0.17 | 2.0 (fixed) |
| 12.91 ± 0.22 | 2.02 ± 0.05 | |
|
|
||
| 0.005 | 12.52 ± 0.22 | 2.0 (fixed) |
| 12.89 ± 0.26 | 1.94 ± 0.06 | |
|
|
||
| 0.010 | 12.33 ± 0.28 | 2.0 (fixed) |
| 12.84 ± 0.63 | 1.93 ± 0.08 | |
|
|
||
| 0.030 | 12.29 ± 0.30 | 2.0 (fixed) |
| 12.91 ± 0.72 | 2.02 ± 0.12 | |
|
|
||
| 0.050 | 11.73 ± 0.65 | 2.0 (fixed) |
| 12.88 ± 0.76 | 1.90 ± 0.14 | |
Notes. We quote the (1) redshift uncertainty; (2) the correlation length r0; (3) slope γ. The mass cut used is Mhalo> 5 × 1013h-1M⊙ and the fit range is fixed at 5–50 Mpc. The fits have been performed both with fixed (γ = 2.0) and free slope.
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