Fig. 10
MCMC posterior distributions of the RV semi-amplitudes for each planet fixing the remaining orbital parameters with the values from Table 5 obtained with Pyaneti. Each of the 180,000 independent Keplerian fits have been tested for 1 Myr dynamical stability using the MVS integrator. Stable solutions are shown in light red. The upper panels of the corner plot show the probability density distributions of each fitted parameter and their mean and 1σ uncertainties in vertical dashed lines.
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.