Table C.2.
Biases induced in the wCDM parameters, using a Gaussian covariance, from neglecting the two studied corrections, for lower and higher fiducial values of σ8 and ns, (0.716, 0.916) and (0.86, 1.06) respectively, are shown.
| Cosmological | EC19 | Low σ8 | High σ8 | Low ns | High ns |
|---|---|---|---|---|---|
| parameter | bias/σ | bias/σ | bias/σ | bias/σ | bias/σ |
| Ωm | −0.51 | −0.33 | −0.76 | −0.70 | −0.41 |
| Ωb | −0.19 | −0.097 | −1.29 | −0.22 | −0.23 |
| h | 0.059 | 0.076 | −0.24 | 0.10 | 0.018 |
| ns | −0.36 | −0.29 | −0.97 | −0.44 | −0.50 |
| σ8 | 0.37 | 0.28 | 0.41 | 0.54 | 0.20 |
| ΩDE | 1.36 | 0.89 | 2.07 | 1.31 | 1.43 |
| w0 | −0.66 | −0.41 | −0.99 | −0.67 | −0.62 |
| wa | 1.21 | 0.76 | 1.85 | 1.15 | 1.26 |
Notes. The biases obtained with the fiducial cosmology of Euclid Collaboration et al. (2019, EC19) are shown for reference.
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