Table 1
Parameters of the flat ΛCDM cosmological model used for the production and analysis of the mock spectra and the CMB-based flat ΛCDM model from Planck Collaboration XIII (2016) used for the analysis of the data.
| Mocks | Planck | |
| (TT+lowP) | ||
|
|
||
| ΩMh2 | 0.1323 | 0.1426 |
| =ΩCh2 | 0.1096 | 0.1197 |
| + ΩBh2 | 0.0227 | 0.02222 |
| + Ωνh2 | 0 | 0.0006 |
| h | 0.7 | 0.6731 |
| N ν | 3 | 3 |
| σ 8 | 0.795 | 0.829 |
| n s | 0.97 | 0.9655 |
|
|
||
| ΩM | 0.27 | 0.3147 |
| rd [Mpc] | 149.7 | 147.33 |
| (104.80 h-1) | (99.17 h-1) | |
| DM(2.33) /rd | 38.63 | 39.15 |
| DH(2.33) /rd | 8.744 | 8.612 |
Notes. The models are defined by the cold dark matter, baryon, and massive neutrinos densities, the Hubble constant, the number of light neutrino species, and the inhomogeneity parameters, σ8 and ns. The sound horizon, rd, is calculated using CAMB (Lewis et al. 2000).
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