Free Access
Fig. 1
Derived posterior probability distributions for the stellar rotation period for two examples: HD 179079 where the rotation period is well determined, and HD 43587 where the rotation period is longer than 29.13 days at 3σ.
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.