Open Access

Fig. 4.

image

Download original image

Comparison of cosmological parameter posterior distributions derived with Commander3 (blue), Python (red), and Cobaya (gray) for a simulation with uniform noise and full-sky coverage. They are made from a single chain per code, and the true input cosmological parameter values are indicated by vertical and horizontal dashed lines.

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.