Table 1.
Parameters and priors considered in the cosmological analyses.
| Parameter | Description | Prior |
|---|---|---|
| Ωm | Total matter density parameter | [0.1, 0.8] |
| σ8 | Amplitude of the power spectrum on the scale of 8 Mpc h−1 | [0.4, 1.6] |
| Ωb | Baryon density parameter | 0.48254 |
| ns | Primordial spectral index | 0.96 |
| h | Normalised Hubble constant | 0.6777 |
| ΣNLk | Non-linear damping at BAO scale | [0, 100] |
| 𝒮k | Extra shot noise parameter | [−3αk, +3αk] |
Notes. The square brackets delimit the intervals of the uniform priors, while the fixed numbers indicate which of the cosmological parameters are assumed to be constant. The extra shot noise term, 𝒮k, is a free parameter only for the angular power spectrum analysis. The normalised Hubble constant, h, is defined as H0/(100 km s−1 Mpc−1).
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