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Table 3

Properties of the selected VIPERS sub-samples in threshold stellar mass bins.

Redshift Median Stellar mass range Median stellar mass N gal r 0 γ Bias γ C BiasC
range redshift [h-2 M] [h-2 M] [h-1 Mpc ]

[0.5, 0.7] 0.61 > 9.0 9.82 17 100 4.55 ± 0.22 1.69 ± 0.05 1.38 ± 0.14 4.99 1.70 1.48
[0.5, 0.7] 0.62 > 9.5 10.11 11 567 5.14 ± 0.25 1.76 ± 0.05 1.50 ± 0.15 5.70 1.77 1.63
[0.5, 0.7] 0.62 > 10.0 10.35 6880 5.84 ± 0.28 1.83 ± 0.05 1.66 ± 0.16 6.01 1.83 1.70
[0.5, 0.7] 0.62 > 10.5 10.66 2151 6.97 ± 0.37 1.86 ± 0.06 1.94 ± 0.17 6.97 1.86 1.94

[0.7, 0.9] 0.78 > 9.0 9.93 15 019 4.53 ± 0.25 1.66 ± 0.04 1.49 ± 0.14 4.73 1.67 1.54
[0.7, 0.9] 0.79 > 9.5 10.15 11 345 4.92 ± 0.26 1.67 ± 0.04 1.59 ± 0.14 5.41 1.69 1.71
[0.7, 0.9] 0.79 > 10.0 10.39 6884 5.37 ± 0.29 1.72 ± 0.04 1.70 ± 0.15 5.87 1.73 1.83
[0.7, 0.9] 0.79 > 10.5 10.67 2498 7.08 ± 0.38 1.73 ± 0.05 2.14 ± 0.18 7.22 1.73 2.18

[0.9, 1.1] 0.97 > 9.5 10.19 4558 4.48 ± 0.21 1.60 ± 0.04 1.66 ± 0.12 4.51 1.62 1.65
[0.9, 1.1] 0.97 > 10.0 10.46 2857 5.57 ± 0.27 1.62 ± 0.04 1.96 ± 0.15 5.78 1.65 2.00
[0.9, 1.1] 0.97 > 10.5 10.71 1281 6.52 ± 0.35 1.74 ± 0.05 2.24 ± 0.18 6.78 1.76 2.30

Notes. The quantities , γC, and biasC are the clustering normalization, slope, and linear bias corrected for the stellar mass incompleteness, respectively. The other parameters and errors are the same as in Table 1.

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