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Table B.1.

Specifics of the most representative galaxy samples.

split centrals centrals + satellites

Ngal/106 b seff Ψ ¯ 0 NFW / c 2 × 10 6 $ \overline{\Psi}^{\mathrm{NFW}}_0/c^2 \times 10^6 $ Ngal/106 b seff Ψ ¯ 0 NFW / c 2 × 10 6 $ \overline{\Psi}^{\mathrm{NFW}}_0/c^2 \times 10^6 $

z ¯ = 1.0 $ \bar{z} = 1.0 $
faint 90% 2.89 1.42 ± 0.02 0.68 ± 0.02 −3.38 3.25 1.55 ± 0.02 0.72 ± 0.03 −3.76
bright 10% 0.321 2.30 ± 0.04 1.44 ± 0.06 −11.5 0.361 2.42 ± 0.04 1.45 ± 0.05 −11.7

faint 50% 1.61 1.25 ± 0.01 0.62 ± 0.03 −2.23 / / / /
bright 50% 1.61 1.75 ± 0.03 0.89 ± 0.04 −6.15 / / / /

z ¯ = 1.2 $ \bar{z} = 1.2 $

faint 90% 2.10 1.65 ± 0.03 0.76 ± 0.03 −4.13 2.48 1.79 ± 0.03 0.80 ± 0.03 −4.55
bright 10% 0.234 2.66 ± 0.05 1.54 ± 0.08 −12.8 0.275 2.78 ± 0.05 1.55 ± 0.06 −12.9

faint 50% 1.17 1.46 ± 0.03 0.68 ± 0.03 −2.86 / / / /
bright 50% 1.17 2.04 ± 0.03 0.99 ± 0.02 −7.14 / / / /

z ¯ = 1.4 $ \bar{z} = 1.4 $

faint 90% 1.55 2.0 ± 0.03 0.83 ± 0.03 −4.66 1.81 2.13 ± 0.03 0.87 ± 0.03 −5.03
bright 10% 0.172 3.19 ± 0.07 1.46 ± 0.4 −13.9 0.201 3.24 ± 0.06 1.46 ± 0.05 −13.8

faint 50% 0.859 1.79 ± 0.03 0.71 ± 0.04 −3.30 / / / /
bright 50% 0.859 2.43 ± 0.04 1.05 ± 0.03 −7.87 / / / /
z ¯ = 1.65 $ \bar{z} = 1.65 $

faint 90% 1.53 2.36 ± 0.04 0.89 ± 0.02 −6.16 1.78 2.59 ± 0.04 0.92 ± 0.03 −6.50
bright 10% 0.170 3.61 ± 0.08 1.6 ± 0.1 −15.4 0.197 3.70 ± 0.08 1.60 ± 0.07 −15.2

faint 50% 0.849 2.11 ± 0.04 0.72 ± 0.04 −4.55 / / / /
bright 50% 0.849 2.85 ± 0.05 1.18 ± 0.05 −9.62 / / / /

Notes. Biases were measured in real space and neglect flux magnification. We report the dimensionless quantity Ψ ¯ 0 NFW / c 2 $ \overline{\Psi}^{\mathrm{NFW}}_0/c^2 $, where Ψ ¯ 0 NFW $ \overline{\Psi}^{\mathrm{NFW}}_0 $ corresponds to the mean value of NFW potential at the galaxy positions for the selected objects. We did not consider the split (50% faint, 50% bright) for the case ‘centrals + satellites’.

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