Table 1
Properties of the selected VIPERS sub-samples in threshold luminosity bins.
Redshift | Median | Magnitude range | Median magnitude | N gal | r 0 | γ | Bias |
range | redshift | MB(z = 1.1) − 5log (h) | MB − 5log (h) | [h-1 Mpc ] | |||
|
|||||||
[0.5, 0.7] | 0.62 | < − 19.5 | −19.87 | 17 473 | 4.45 ± 0.20 | 1.67 ± 0.05 | 1.36 ± 0.13 |
[0.5, 0.7] | 0.62 | < − 20.0 | −20.15 | 12 432 | 4.81 ± 0.21 | 1.69 ± 0.05 | 1.44 ± 0.14 |
[0.5, 0.7] | 0.62 | < − 20.5 | −20.49 | 7472 | 5.22 ± 0.29 | 1.73 ± 0.06 | 1.53 ± 0.17 |
[0.5, 0.7] | 0.62 | < − 21.0 | −20.86 | 3599 | 5.58 ± 0.39 | 1.81 ± 0.08 | 1.60 ± 0.19 |
[0.5, 0.7] | 0.62 | < − 21.5 | −21.28 | 1236 | 6.24 ± 0.56 | 1.79 ± 0.14 | 1.73 ± 0.24 |
|
|||||||
[0.7, 0.9] | 0.79 | < − 20.0 | −20.41 | 14 442 | 4.56 ± 0.22 | 1.65 ± 0.04 | 1.50 ± 0.12 |
[0.7, 0.9] | 0.80 | < − 20.5 | −20.68 | 9469 | 4.95 ± 0.23 | 1.67 ± 0.04 | 1.59 ± 0.11 |
[0.7, 0.9] | 0.80 | < − 21.0 | −21.05 | 4605 | 5.32 ± 0.30 | 1.70 ± 0.05 | 1.67 ± 0.12 |
[0.7, 0.9] | 0.80 | < − 21.5 | −21.45 | 1619 | 5.95 ± 0.39 | 1.72 ± 0.10 | 1.79 ± 0.15 |
|
|||||||
[0.9, 1.1] | 0.97 | < − 20.5 | −21.00 | 5207 | 4.29 ± 0.19 | 1.63 ± 0.04 | 1.58 ± 0.11 |
[0.9, 1.1] | 0.98 | < − 21.0 | −21.25 | 3477 | 5.08 ± 0.26 | 1.64 ± 0.05 | 1.79 ± 0.12 |
[0.9, 1.1] | 0.99 | < − 21.5 | −21.65 | 1409 | 5.87 ± 0.43 | 1.68 ± 0.08 | 2.04 ± 0.19 |
Notes. The best-fit values of the clustering normalization, r0, and slope, γ, have been obtained by fitting wp(rp) in 0.2 < rp [h-1 Mpc ] < 20. The errors are from the scatter among the HOD VIPERS mocks. The bias values assume a flat ΛCDM model with ΩM = 0.25 and σ8 = 0.8.
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