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Fig. 6

image

Posterior distribution of the second companion minimum mass as a function of its orbital period, assuming a circular orbit. The three regions represent the 68.3%, 95.5%, and 99.7% confidence intervals from the MCMC analysis (from dark to light grey). The dashed line indicates the planet – brown dwarf limit as suggested by Schneider et al. (2011). The solid line indicates the hydrogen-burning limit.

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