Free Access
Fig. 9
Radial velocity of the planet as a function of orbital phase. It is obtained by fitting the average Fe II line as a Gaussian in each exposure of each of the two nights. The blue line signifies our fit of Eq. (7), which yields a best-fit projected orbital velocity of 234.24 ± 0.90 km s−1.
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.