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Table 2
Best-fit cosmological parameters for various combinations of data and analysis methods.
| Data | σ8(Ωm/ 0.27)0.3 | Ωm | σ 8 | 1 − b |
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| Planck SZ and BAO and BBN | 0.764 ± 0.025 | 0.29 ± 0.02 | 0.75 ± 0.03 | [0.7, 1] |
| Planck SZ and HST and BBN | 0.774 ± 0.024 | 0.28 ± 0.03 | 0.77 ± 0.03 | [0.7, 1] |
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| Planck SZ and BAO and BBN | 0.782 ± 0.010 | 0.29 ± 0.02 | 0.77 ± 0.02 | 0.8 |
| MMF1 sample and BAO and BBN | 0.800 ± 0.010 | 0.29 ± 0.02 | 0.78 ± 0.02 | 0.8 |
| MMF3 S/N > 8 and BAO and BBN | 0.785 ± 0.011 | 0.29 ± 0.02 | 0.77 ± 0.02 | 0.8 |
| Planck SZ and BAO and BBN (MC completeness) | 0.778 ± 0.010 | 0.30 ± 0.03 | 0.75 ± 0.02 | 0.8 |
| Planck SZ and BAO and BBN (Watson et al. mass function) | 0.802 ± 0.014 | 0.30 ± 0.01 | 0.77 ± 0.02 | 0.8 |
Notes. For the analysis using the Watson et al. mass function, or (1 − b) in [ 0.7,1 ], the degeneracy line is different, and thus the value of σ8(Ωm/ 0.27)0.3 is just illustrative.
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