Table B.1.
Values of the halo mass cut (Mcut in units of 1014 M⊙), and mass–richness fit parameters lnA, β, and σ (as in of Eq. 4) for each simulation used in this work.
| z = 0.00 | z = 0.14 | z = 0.29 | z = 0.47 | |||||||||||||
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| Mcut | lnA | β | σ | Mcut | lnA | β | σ | Mcut | lnA | β | σ | Mcut | lnA | β | σ | |
| C1 | - | - | - | - | - | - | - | - | - | - | - | - | - | - | - | - |
| C2 | 15.2 | −0.76 | 1.76 | 1.39 | 4.0 | 0.72 | 0.87 | 0.06 | - | - | - | - | - | - | - | - |
| C3 | 4.8 | 0.73 | 1.05 | 0.03 | 4.5 | 0.87 | 0.98 | 0.04 | 4.5 | 0.98 | 0.98 | 0.04 | 5.0 | 1.05 | 0.88 | 0.05 |
| C4 | 9.6 | 0.25 | 1.20 | 0.14 | 9.7 | 0.69 | 0.83 | 0.16 | - | - | - | - | 6.6 | 0.85 | 0.76 | 0.24 |
| C5 | 8.4 | 0.49 | 1.01 | 0.08 | 7.1 | 0.50 | 1.15 | 0.07 | 9.6 | 0.49 | 1.23 | 0.10 | 7.5 | 0.33 | 1.45 | 0.10 |
| C6 | 11.0 | −0.41 | 1.62 | 0.33 | - | - | - | - | 7.8 | −0.04 | 1.71 | 0.22 | - | - | - | - |
| C7 | 16.3 | −0.88 | 1.62 | 1.40 | 6.0 | 0.61 | 0.83 | 0.07 | 6.1 | 0.84 | 0.72 | 0.09 | 5.7 | 0.84 | 0.52 | 0.11 |
| C8 | 4.3 | 0.78 | 0.98 | 0.03 | 4.8 | 0.93 | 0.90 | 0.03 | 5.1 | 1.01 | 0.89 | 0.03 | 4.6 | 1.04 | 1.01 | 0.04 |
| C9 | 7.9 | 0.60 | 0.99 | 0.04 | 8.1 | 0.63 | 1.08 | 0.04 | 7.1 | 0.87 | 0.86 | 0.04 | 7.0 | 0.87 | 0.97 | 0.06 |
| C10 | 4.8 | 0.73 | 1.02 | 0.02 | 4.0 | 0.88 | 1.00 | 0.02 | 3.6 | 0.99 | 1.02 | 0.02 | 4.5 | 1.13 | 0.94 | 0.02 |
| C11 | 7.4 | 0.47 | 1.01 | 0.03 | 7.3 | 0.65 | 0.93 | 0.02 | 5.4 | 0.70 | 0.92 | 0.04 | 7.3 | 0.63 | 1.13 | 0.05 |
| C12 | 4.8 | 0.56 | 1.00 | 0.02 | 6.1 | 0.70 | 0.98 | 0.02 | 7.1 | 0.83 | 0.95 | 0.03 | 5.9 | 0.85 | 1.02 | 0.04 |
| C13 | - | - | - | - | - | - | - | - | - | - | - | - | - | - | - | - |
| C14 | 10.4 | 0.18 | 1.06 | 0.03 | 9.4 | 0.31 | 1.04 | 0.03 | 7.6 | 0.38 | 1.02 | 0.03 | 10.2 | 0.24 | 1.33 | 0.07 |
| C15 | 9.4 | 0.23 | 1.01 | 0.03 | 9.2 | 0.44 | 0.91 | 0.04 | 9.6 | 0.28 | 1.14 | 0.04 | 10.5 | 0.55 | 0.92 | 0.09 |
Notes. Each row corresponds to a given cosmology C1–C15, column-groups report redshift slices. Cells containing a dash report cosmology–redshift configurations for which the setups had an insufficient number of haloes within the mass cut, as explained in Sect. 4.2.
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