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Table 7.
Relative errors on the cosmological parameter constraints between the M1 and M2 approaches (both with optimal step sizes) after projection to the θcosmo parameter set.
| Parameter | Relative error (%) |
|---|---|
| Ωb | 1.857e−3 |
| h | 2.332e−3 |
| Ωm | −2.176e−2 |
| ns | 2.155e−2 |
| ΩDE | −1.137e−3 |
| w0 | −7.339e−3 |
| wa | −1.573e−3 |
| σ8 | −5.706e−3 |
Notes. In both cases, the covariance matrices are marginalized over the nuisance parameters.
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