Fig. 3
Probability distribution (see Table 4 for details) of the frequency of planetary mass (up to 15 MJup, left panels) and BD (16−70 MJup, right panels). The results for the CBIN sample and the and the SS control sample are shown in the upper and lower panels, respectively. The shaded areas show the frequency limits for the 95% (gray) and 68% (blue) confidence levels.
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