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Table 1.
Prior ranges of cosmological and nuisance parameters in the likelihood analysis.
| Parameter | Prior Type | Prior range |
|---|---|---|
| Ωm | uniform | [0.1, 0.55] |
| h | uniform | [0.6, 0.82] |
| Ωb | delta | 0.0447 |
| τ | delta | 0.08 |
| ns | delta | 0.969 |
| σ8 | uniform | [0.53, 1.3] |
| w0 | uniform | [ − 2.0, −0.5] |
| wa | delta | 0 |
| S8 | uniform | [0.6, 0.9] |
| AIA | uniform | [ − 5, 5] |
| baryon feedback | uniform | [0, 2] |
| Δm1 | Gaussian | μ = 0.12, σ = 0.023 |
| Δm2 | Gaussian | μ = 0.12, σ = 0.023 |
| Δm3 | Gaussian | μ = 0.12, σ = 0.023 |
| Δm4 | Gaussian | μ = 0.12, σ = 0.023 |
| dz1 | Gaussian | μ = 0, σ = 0.008 |
| dz2 | Gaussian | μ = 0, σ = 0.014 |
| dz3 | Gaussian | μ = 0, σ = 0.011 |
| dz4 | Gaussian | μ = 0, σ = 0.009 |
Notes. Priors on cosmological parameters are provided by the range of our Cosmology Training Set, prior on Δmi and on AIA are from T+18, while those on dzi are from Joudaki et al. (2020).
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