Table 1.
Prior ranges used in the Planck-18 TTTEEE and KiDS-1000 analysis.
| Parameters | Symbol | Prior |
|---|---|---|
| Cold DM energy density | ωcdm | [0.051, 0.255] |
| Baryon energy density | ωb | [0.019, 0.026] |
| Initial P(k) amplitude | log(1010As) | [1.0, 5.0] |
| Hubble constant | h | [0.5, 0.9] |
| Spectral index | ns | a[0.8, 1.3] |
| Optical depth | τ | 𝒩(0.0544, 0.007) |
| Intrinsic alignment amplitude | AIA | [−2, 2] |
| First gas parameter (lmttBCemu) | log10(Mc) | [11.0, 15.0] |
| Second gas parameter (lmttBCemu) | θj | [4.0, 6.0] |
| Stellar parameter (lmttBCemu) | ηδ | [0.05, 0.40] |
| HDM fraction | fhdm | [0.0, 1.0] |
| Thermal mass | log10(1/mhdm(keV)) | [−0.17, 2.00] |
Notes. We used flat priors for all the parameters excluding τ, which has a Gaussian prior to recover the posteriors of the uncompressed analysis as explained in Prince & Dunkley (2019). Horizontal lines distinguish: (I) standard ΛCDM parameters, (II) CMB only parameters, (III) KiDS-1000 parameters, and (IV) MDM extension parameters.
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