Table 5
Estimates of cosmological parameters using MCMC techniques for the six ΛCDM parameters.
Parameter | Hillipop+lowTEB | Hillipop+lowTEB | Hillipop+lowTEB |
+ VHL | + VHL + BAO + SN | ||
|
|||
Ωbh2 ............... | 0.02220 ± 0.00023 | 0.02203 ± 0.00020 | 0.02211 ± 0.00018 |
Ωch2 ............... | 0.1193 ± 0.0022 | 0.1196 ± 0.0020 | 0.1183 ± 0.0012 |
100θs ............... | 1.04179 ± 0.00043 | 1.04181 ± 0.00042 | 1.04190 ± 0.00038 |
τ .............................. | 0.071 ± 0.019 | 0.058 ± 0.018 | 0.062 ± 0.017 |
ns .............................. | 0.9644 ± 0.0069 | 0.9626 ± 0.0055 | 0.9654 ± 0.0040 |
ln(1010As) ............... | 3.068 ± 0.037 | 3.044 ± 0.034 | 3.048 ± 0.033 |
|
|||
H0 .............................. | 67.48 ± 0.98 | 67.21 ± 0.91 | 67.77 ± 0.57 |
σ8 .............................. | 0.816 ± 0.015 | 0.809 ± 0.013 | 0.807 ± 0.013 |
Notes. First with our likelihood (Hillipop) and lowTEB. Then with our regularized likelihood (Hillipop+lowTEB+VHL, second column) and further adding some BAO and SN data (third column). Here θs, as computed by class, represents the exact angular size of the sound horizon and should not be identified with the CosmoMCθMC parameter (see Appendix B).
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