Fig. 3
Download original image
HARPS RV residuals Keplerian and GP model fit. Top: HARPS RV residuals after fitting CORALIE and HARPS data with a two-planet plus trend model described in Sect. 3.2.2 with a one-planet Keplerian plus GP model constrained by the HARPS RV and BIS. Middle: GP fit to the HARPS BIS data. Bottom: HARPS RV residuals from the top phased to the 1-day planet 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.