Free Access
Fig. 10
Probability of observing N planets with periods up to 50 days in a simulated system, formed through either pebble or planetesimal accretion. We show the probabilities for both the transit method, assuming that only planets with masses, mp > 0.1 M⊕ may be observed, and the RV method, assuming a detection limit of 1 m 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.