Free Access

Fig. 8

thumbnail

Top: joint probability density function of the orbital period and the eccentricity. The red (resp. blue, cyan) line corresponds to the 1 (resp. 2, 3)σ confidence interval. Bottom: minimum mass distribution of the planetary companions with the same confidence intervals. 99.73% of the solutions have a period between 5 and 90 years, an eccentricity between 0.47 and 0.95 and a minimum mass between 3.5 and 15 MJup.

This figure is made of several images, please see below:

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.