Fig. 8
Difference in RV measurement from the average for faint stars in the sample vs. the square of the S/N at 550 nm, a quantity that is roughly proportional to the flux recorded in the spectra. No trend is visible, and this indicates that if detector charge transfer inefficiency is present, it does not affect our measurements in a detectable way.
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.