Open Access
Table 1.
Different cosmological parameters considered in this work.
Name | Ωm, 0 | h | Ωb, 0 | ns | σ8 |
---|---|---|---|---|---|
C0 | 0.3158 | 0.6732 | 0.0494 | −0.9661 | 0.8102 |
C1 | 0.1986 | 0.7267 | 0.0389 | −0.9775 | 0.8590 |
C2 | 0.1665 | 0.7066 | 0.0417 | −0.9461 | 0.8341 |
C3 | 0.3750 | 0.6177 | 0.0625 | −0.9778 | 0.7136 |
C4 | 0.3673 | 0.6353 | 0.0519 | −0.9998 | 0.7121 |
C5 | 0.1908 | 0.6507 | 0.0527 | −0.9908 | 0.8971 |
C6 | 0.2401 | 0.8087 | 0.0357 | −0.9475 | 0.8036 |
C7 | 0.3020 | 0.5514 | 0.0674 | −0.9545 | 0.8163 |
C8 | 0.4093 | 0.7080 | 0.0446 | −0.9791 | 0.7253 |
Notes. The cosmological parameters have been uniformly drawn from the 95 percent confidence level hyper-volume of the cluster abundance constraints presented in Costanzi et al. (2021).
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