Table 3
Richness results for different redshift intervals.
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Nhalos | Log![]() |
z |
(1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) |
|
|||||||
0.19 ± 0.11 | −0.039 ± 0.10 | 0.11 | 0.14 | 0.14 | 179 | 14.01 ± 0.24 | 0.0–0.5 |
0.23 ± 0.13 | −0.0069 ± 0.14 | 0.11 | 0.14 | 0.15 | 175 | 14.00 ± 0.21 | 0.5–0.75 |
0.25 ± 0.14 | −0.0043 ± 0.14 | 0.12 | 0.17 | 0.18 | 245 | 13.90 ± 0.21 | 0.75–1.0 |
0.27 ± 0.15 | 0.0034 ± 0.17 | 0.12 | 0.19 | 0.21 | 229 | 13.84 ± 0.22 | 1.0–1.25 |
0.26 ± 0.14 | −0.017 ± 0.15 | 0.12 | 0.17 | 0.18 | 159 | 13.79 ± 0.19 | 1.25–1.5 |
0.27 ± 0.15 | 0.0050 ± 0.17 | 0.15 | 0.19 | 0.21 | 127 | 13.73 ± 0.20 | 1.5–1.75 |
0.33 ± 0.14 | 0.061 ± 0.17 | 0.13 | 0.14 | 0.17 | 60 | 13.70 ± 0.18 | 1.75–2.0 |
0.29 ± 0.13 | 0.017 ± 0.15 | 0.13 | 0.16 | 0.18 | 33 | 13.68 ± 0.19 | 2.0–2.5 |
Notes. Column description. (1) Mean logarithmic difference between the estimated richness λ1 = Nestimated and the true richness Ntrue, where the reported uncertainty is the rms dispersion around the mean and the richness λ1 = Nestimated refers to galaxies with Pmem>Pthr = 20%; (2) as in Col. 1, but here the estimated richness λ2 = ∑ Pmem is used; (3) rms dispersion around the mean of the logarithmic difference between the halo mass Mhalo and the halo occupation number Ntrue; (4) rms dispersion around the mean of the logarithmic difference between the halo mass Mhalo and the estimated richness λ1 = Nestimated; (5) as in Col. 4, but here the estimated richness λ2 = ∑ Pmem is used; (6) number of halos considered; (7) median logarithmic halo mass, the reported uncertainty is the rms dispersion; (8) redshift bin.
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