Fig. 3
Lomb-Scargle periodogram of the residuals between TESS photometry in orbit 22 and the best-fit model for WASP-121b. The orange dashed line indicates the rotational modulation identified in the RVs at 1.13 d. The peak indicated by the red dashed line at 1.37 d is only present in this orbit, and likely traces a transient active region at higher stellar latitudes.
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.