Table 3.
Summary statistics for the fits of the 25 mocks with spherical full-sky footprint from z = 0.15 to z = 0.25, Planck 2018 cosmology, and the median HOD, where the clustering was measured using cosmology C177 of the ABACUSSUMMIT suite as fiducial cosmology resulting in an isotropic dilatation parameter αv ≈ 1.02.
| MGPαV [ × 10−2] | MGP[ × 10−2] | |||||
|---|---|---|---|---|---|---|
| accounting αV | neglecting for αV | |||||
| p | ⟨Δp⟩ | ⟨σp⟩ | std(p) | ⟨Δp⟩ | ⟨σp⟩ | std(p) |
| f | −0.02 | 0.59 | 0.10 | −0.20 | 0.75 | 0.15 |
| ωm | −0.00 | 0.10 | 0.02 | −0.04 | 0.13 | 0.03 |
| ωb | −0.00 | 0.04 | 0.00 | −0.00 | 0.05 | 0.01 |
| σ8 | −0.04 | 0.19 | 0.01 | −0.04 | 0.23 | 0.02 |
| w0 | −0.13 | 2.93 | 0.28 | −0.03 | 3.27 | 0.41 |
| wa | 0.56 | 11.77 | 0.80 | 0.34 | 12.68 | 1.67 |
| h | 0.02 | 0.42 | 0.08 | 0.15 | 0.52 | 0.09 |
| ns | 0.01 | 0.45 | 0.07 | 0.01 | 0.50 | 0.08 |
| Nur | −1.34 | 30.49 | 2.05 | −2.94 | 31.75 | 5.01 |
| αs | 0.00 | 0.22 | 0.02 | 0.01 | 0.28 | 0.04 |
| α | 5.66 | 32.97 | 5.97 | 10.54 | 23.24 | 4.75 |
| κ | −1.57 | 26.37 | 1.23 | 0.04 | 22.84 | 4.53 |
| logM1 | −0.51 | 32.20 | 3.99 | −1.27 | 30.42 | 8.47 |
| logMcut | 5.06 | 11.15 | 2.09 | 8.95 | 11.12 | 2.87 |
| logσ | 6.96 | 15.94 | 2.92 | 4.74 | 13.97 | 2.56 |
Notes. ⟨Δp⟩ is the bias, the difference between the true and best-fit value for any parameter p, ⟨σp⟩ is the average over the 25 realisations of the (symmetrised) one sigma confidence level, and std(p) is the standard deviation of the estimated parameter p over the 25 results. We note that f is a derived parameter from the other cosmological parameters.
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