Free Access
Fig. 4
Radial-velocity signatures of the four Keplerians fitted to the GJ 676A measurements (top row) and the residuals as a function of respective orbital phase. Black circles with uncertainties show the HARPS measurements and the blue curves indicate the best-fit model.
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.