Table 9.
Shift in best-fit parameters for GCph + WL + GGL.
| Model | Ωm, 0 | Ωb, 0 | w0 | wa | h | ns | σ8 | ∑mν |
|---|---|---|---|---|---|---|---|---|
| ΛCDM | 4.73 | 0.41 | – | – | −0.56 | −1.76 | −2.88 | – |
| ΛCDM + ∑mν | 5.64 | 0.65 | – | – | 0.07 | −1.51 | −4.21 | 3.08 |
| w0 waCDM | 6.90 | 2.89 | 4.58 | −2.82 | 1.16 | −4.39 | −4.56 | – |
| w0 waCDM + ∑mν | 6.21 | 2.71 | 4.57 | −2.82 | 1.09 | −3.60 | −2.91 | 0.51 |
Notes. We report the shift in the values of the best fitting parameters, in units of 1σ, for the same models as in Table 7. The shifts are computed with the formalism described in Sect. 4.2, and therefore, the values of shifts that are larger than 1σ cannot be quantitatively trusted but indicate that the shift is large. We marginalise over the galaxy bias and intrinsic alignment parameters, and the values of the local count slope are fixed to their fiducial values.
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