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Table 1.
Parameters, prior and posterior mean, and percentiles of the cosmological analyses.
| Parameter | Description | Prior w(θ)−Cℓ | Posterior w(θ)−Cℓ |
|---|---|---|---|
| Ωm | Total matter density parameter | [0.1, 0.7] |
 |
| σ8 | Amplitude of the power spectrum on the scale of 8 h−1 Mpc | [0.3, 1.5] |
 |
| S8 ≡ σ8(Ωm/0.3)0.5 | Structure growth parameter | – |
 |
| Ωb | Baryon density parameter | 𝒢(0.0486, 0.0017) | – |
| ns | Primordial spectral index | 𝒢(0.9649, 0.0210) | – |
| h ≡ H0/(100 km s−1 Mpc−1) | Normalised Hubble constant | 𝒢(0.7, 0.1) | – |
| α | Normalisation of the mass-richness scaling relation | 𝒢(0.04, 0.04) | – |
| β | Slope of the mass-richness scaling relation | 𝒢(1.72, 0.08) | – |
| γ | Redshift evolution of the mass-richness scaling relation | 𝒢(−2.37, 0.40) | – |
| σintr, 0 | Normalisation of σintr | 𝒢(0.18, 0.09) | – |
| σintr, λ* | λ* evolution of σintr | 𝒢(0.11, 0.20) | – |
| 𝒮1 | Extra shot noise bin 1 | – 𝒢(0.0, 4.2 × 10−6) | – |
| 𝒮2 | Extra shot noise bin 2 | – 𝒢(0.0, 2.0 × 10−6) | – |
| 𝒮3 | Extra shot noise bin 3 | – 𝒢(0.0, 2.2 × 10−6) | – |
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