MCMC results using the CARMENES RVs obtained for GJ 3779. Each panel contains approximately 40 000 Keplerian samples. The upper panels of the corner plot show the probability density distributions of each orbital parameter. The vertical dashed lines indicate the mean and 1σ uncertainties of the fitted parameters. The rest of the panels show the dependencies between all the orbital elements in the parameter space. Black contours are drawn to improve the visualisation of the two-dimensional histograms. The distributions agree within the errors with the best-fit values from Table 2.