Table 6.
Marginalized 1-σ errors in different cosmological scenarios for WL + V + GCsp, when they are assumed to be independent, together with their combinations when the void-lensing cross-correlation is included.
| Probe | h | Ωm | Ωb | σ8 | ns | Mν [eV] | w0 | wa | FoM |
|---|---|---|---|---|---|---|---|---|---|
| w0waCDM | |||||||||
| 0.00435 | 0.00931 | 0.00301 | 0.00947 | 0.00832 | – | 0.0923 | 0.31 | 113 | |
| WL + V + GCsp | 0.00133 | 0.00395 | 0.00128 | 0.0065 | 0.0036 | – | 0.0256 | 0.196 | 702 |
| 0.00420 | 0.00856 | 0.00295 | 0.0092 | 0.00811 | – | 0.0883 | 0.295 | 124 | |
| WL + V + XC + GCsp | 0.0013 | 0.0018 | 0.00088 | 0.00205 | 0.00332 | – | 0.0228 | 0.113 | 791 |
Notes. In each probe block, the first row shows the errors for the pessimistic scenario, while the second row corresponds to the optimistic one.
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.