Table 8.
Summary of a selection of the cases investigated for the weak-lensing code comparison, ordered according to the number of parameters involved.
| Case | No. of parameters | Parameters |
ℓmax | |||
|---|---|---|---|---|---|---|
| Flat | Non-flat | MG | IA | |||
| 1 | 5 | Ωm, 0 Ωb, 0 h ns σ8 | – | – | – | 1500 or 5000 |
| 2 | 6 | Ωm, 0 Ωb, 0 h ns σ8 | ΩDE, 0 | – | – | 1500 or 5000 |
| 3 | 7 | Ωm, 0 Ωb, 0 w0 wa h ns σ8 | – | – | – | 1500 or 5000 |
| 4 | 8 | Ωm, 0 Ωb, 0 w0 wa h ns σ8 | ΩDE, 0 | – | – | 1500 or 5000 |
| 5 | 8 | Ωm, 0 Ωb, 0 w0 wa h ns σ8 | – | γ | – | 1500 or 5000 |
| 6 | 9 | Ωm, 0 Ωb, 0 w0 wa h ns σ8 | ΩDE, 0 | γ | – | 1500 or 5000 |
| 7 | 10 | Ωm, 0 Ωb, 0 w0 wa h ns σ8 | – | – | 𝒜IA ηIA βIA | 1500 or 5000 |
| 8 | 11 | Ωm, 0 Ωb, 0 w0 wa h ns σ8 | ΩDE, 0 | – | 𝒜IA ηIA βIA | 1500 or 5000 |
| 9 | 11 | Ωm, 0 Ωb, 0 w0 wa h ns σ8 | – | γ | 𝒜IA ηIA βIA | 1500 or 5000 |
| 10 | 12 | Ωm, 0 Ωb, 0 w0 wa h ns σ8 | ΩDE, 0 | γ | 𝒜IA ηIA βIA | 1500 or 5000 |
Notes. In non-flat cases, ΩDE, 0 is included as a free cosmological parameter (or equivalently ΩK, 0). The quantity ℓmax is the maximum multipole included in the analysis. MG corresponds to the modified gravity γ parameter (see Eq. (32)), changing the growth of structure. IA refers to intrinsic alignment parameters (discussed in Sect. 3.3.1).
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.