Table 3.
Priors considered in the various redshift and amplitude bins.
| − | log M200 | c200 | foff | σoff | ΩM |
|---|---|---|---|---|---|
| 1 | 13.170 ± 0.088 | 9.3 ± 5.2 | 0.25 ± 0.14 | 0.22 ± 0.13 | [0.06−0.6] |
| 2 | 13.517 ± 0.074 | 7.4 ± 4.6 | 0.28 ± 0.14 | 0.26 ± 0.13 | " " |
| 3 | 14.034 ± 0.059 | 2.7 ± 1.3 | 0.27 ± 0.14 | 0.24 ± 0.14 | " " |
| 4 | 14.214 ± 0.067 | 3.6 ± 2.0 | 0.28 ± 0.14 | 0.26 ± 0.14 | " " |
| 5 | 14.507 ± 0.065 | 5.2 ± 2.1 | 0.31 ± 0.14 | 0.20 ± 0.10 | " " |
| 6 | 13.579 ± 0.069 | 12.1 ± 4.5 | 0.22 ± 0.14 | 0.23 ± 0.15 | " " |
| 7 | 13.835 ± 0.073 | 4.2 ± 3.1 | 0.29 ± 0.14 | 0.29 ± 0.13 | " " |
| 8 | 14.176 ± 0.059 | 2.3 ± 1.1 | 0.28 ± 0.14 | 0.26 ± 0.13 | " " |
| 9 | 14.255 ± 0.082 | 12.0 ± 4.5 | 0.24 ± 0.14 | 0.26 ± 0.15 | " " |
| 10 | 14.557 ± 0.074 | 9.3 ± 4.3 | 0.26 ± 0.14 | 0.24 ± 0.14 | " " |
| 11 | 13.664 ± 0.088 | 7.5 ± 4.8 | 0.29 ± 0.14 | 0.24 ± 0.12 | " " |
| 12 | 13.837 ± 0.069 | 10.7 ± 4.6 | 0.25 ± 0.14 | 0.22 ± 0.13 | " " |
| 13 | 14.143 ± 0.082 | 4.9 ± 3.4 | 0.29 ± 0.14 | 0.29 ± 0.14 | " " |
| 14 | 14.345 ± 0.082 | 5.7 ± 3.6 | 0.29 ± 0.14 | 0.25 ± 0.13 | " " |
Notes. The different lines are ordered as in Table 1. For the halo structural properties (first four columns) we consider Gaussian priors with mean and standard deviations derived from the posteriors of the ∼1h case analysis, while for the total matter density parameter (last column) we assume a uniform prior.
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