Mean of the CCFs observed outside of the transit in Run 2012, as a function of radial velocities relative to the star. Before calculating the average, the CCFs in each run were shifted from the velocity frame of the solar system barycenter where they are computed, to the frame of KOI-12 using the best-fit systemic velocities derived in Sect. 5.1. Note the strong tilt of the asymmetric continuum.
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.