Table 1.
Cosmological parameters of the simulations used in this work.
| h | Ωm | Ωb | σ8 | ns | |
|---|---|---|---|---|---|
| TheOne | 0.680 | 0.307 | 0.0480 | 0.900 | 0.960 |
| D3A | 0.681 | 0.306 | 0.0486 | 0.807 | 0.967 |
| LS8 | 0.682 | 0.305 | 0.0473 | 0.760 | 0.965 |
| Planck | 0.673 | 0.316 | 0.0494 | 0.812 | 0.966 |
| WMAP9 | 0.700 | 0.279 | 0.0460 | 0.820 | 0.970 |
Notes. The table reports the cosmologies of the simulations used in this work. “TheOne” is from the BACCO simulation suite. “D3A” corresponds to the FLAMINGO simulation run with the DES Y3 “3 × 2pt+ All Ext”. ΛCDM cosmology (DES Collaboration 2022). “LS8” refers to a FLAMINGO run with low σ8, and “Planck” uses the Planck Collaboration VI (2020) cosmology. The Takahashi simulations adopt a cosmology approximately consistent with WMAP9 (Hinshaw et al. 2013). The parameters shown are: the dimensionless Hubble parameter h, the matter and baryon density parameters Ωm and Ωb, the amplitude of linear fluctuations σ8, and the spectral index ns.
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