Table 1
Change of cosmic shear bispectrum statistical power after nulling (null) and linear data compression (compress).
| i | Null | Null/i | Compress | Compress/i | |
|
|
|||||
| Ωm − σ8 | 21455 | 4609 | 21.5% | 12242 | 57.1% |
| Ωm − w0 | 637 | 123 | 19.3% | 428 | 67.2% |
| Ωm − wa | 145 | 33 | 23.0% | 110 | 75.9% |
| σ8 − w0 | 434 | 87 | 20.0% | 299 | 68.9% |
| σ8 − wa | 101 | 26 | 25.4% | 72 | 71.3% |
| w0 − wa | 11.4 | 2.3 | 20.2% | 8.0 | 70.2% |
Notes. Presented are FoM on two-dimensional parameter planes between cosmological parameters Ωm, σ8, w0 and wa. The cosmological parameters h, Ωb and ns are marginalized over. The second column is the FoM from the original bispectrum; the third and fifth columns are FoM from the nulled and the compressed measures, respectively; the fourth (sixth) column shows the percentage of the third (fifth) column compared to the first column, which reflects the relative information loss through the nulling (the unconditioned compression) procedure.
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.