Table 6.
Shift in best-fit parameters for GCph alone.
| Model | Ωm, 0 | Ωb, 0 | w0 | wa | h | ns | σ8 | ∑mν |
|---|---|---|---|---|---|---|---|---|
| ΛCDM | −0.18 | 0.004 | – | – | −0.02 | 0.33 | −0.57 | – |
| ΛCDM + ∑mν | 0.96 | −0.15 | – | – | −0.42 | 0.98 | −1.62 | 1.64 |
| w0 waCDM | −0.65 | −0.64 | −1.02 | 1.20 | 0.05 | 1.04 | 0.17 | – |
| w0 waCDM + ∑mν | −0.90 | −1.12 | −1.27 | 1.21 | 0.22 | 1.59 | −0.13 | 1.62 |
Notes. The shift in best-fit parameters are in units of 1σ. We report the results for the same models as in Tables 3 and 4. The shifts are estimated with the formalism described in Sect. 4.2. The values of shifts that are larger than 1σ cannot be trusted but indicate that the shift is large. We marginalise over the galaxy bias parameters, and the values of the local count slope are fixed to their fiducial values.
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