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Table 1.
ΛCDM cosmological parameters adopted in this work, corresponding to the best-fit cosmology from Planck Collaboration I (2020), and the KiDS-1000 multivariate maximum posterior (MAP) results from the two-point correlation functions ξ±, the band powers C(ℓ), and the COSEBIs, as in Asgari et al. (2021).
| Survey | h0 | Ωbh2 | Ωch2 | ns | σ8 |
|---|---|---|---|---|---|
| Planck | 0.673 | 0.022 | 0.120 | 0.966 | 0.812 |
| KiDS ξ± | 0.711 | 0.023 | 0.088 | 0.928 | 0.895 |
| KiDS C(ℓ) | 0.704 | 0.022 | 0.132 | 0.999 | 0.723 |
| KiDS COSEBI | 0.727 | 0.023 | 0.105 | 0.949 | 0.772 |
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