Free Access

Fig. A.3.

image

Constraints on sampled cosmological and astrophysical parameters. Results are shown for COSEBIs (orange), band powers (pink) and the 2PCFs (cyan). We use kernel density estimation to smooth the distributions, which in the case of poorly constrained parameters can produce artificial constraints near the prior boundaries (for example constraints on h or Ωbh2).

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.