Fig. 12
Posterior probability distribution of the frequency of planetary mass (2–15 MJup; top panels) and BDs (16-70 MJup; bottom panels). The results of the SPOTS II dataset alone and the combined 163 SPOTS II + III targets are shown on the left and right columns, respectively. The 95 (light grey) and 68% (dark grey) confidence levels are shown as shaded areas.
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