Table 1
Parameters of the flat-ΛCDM cosmological model used for the production and analysis of the mock spectra and for the analysis of the data.
| Mocks | Planck | |
| (TT + lowP) | ||
|
|
||
| Ωmh2 | 0.1323 | 0.1426 |
| = Ωch2 | 0.1090 | 0.1197 |
| + Ωbh2 | 0.0227 | 0.02222 |
| + Ωνh2 | 0.0006 | 0.0006 |
| h | 0.7 | 0.6731 |
| N ν | 3 | 3 |
| σ 8 | 0.795 | 0.830 |
| n s | 0.97 | 0.9655 |
|
|
||
| Ωm | 0.27 | 0.3147 |
| rd [h-1 Mpc] | 104.80 | 99.17 |
| rd [Mpc] | 149.7 | 147.33 |
| z eff | 2.25 | 2.40 |
| DH(zeff) /rd | 8.495 | 8.369 |
| DM(zeff) /rd | 39.24 | 39.77 |
| f(zeff) | 0.95916 | 0.97076 |
Notes. The Planck Collaboration XIII (2016) cosmological parameters are used for the data. The parameters defining the models are given in the first section: the density of cold dark matter, baryon, and massive neutrinos, the reduced Hubble constant, and the number of light neutrino species. The second section of the table gives derived parameters and quantities calculated at the relevant redshift zeff. The sound horizon at the drag epoch, rd, is calculated using CAMB (Lewis et al. 2000). The linear growth rate of structure is calculated using the approximation f ~ Ωm(z)0.55 (Linder & Cahn 2007).
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