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Caption: Figure 5.
The eccentricity as a function of the period for published brown-dwarf-hosting systems. Gray triangles denote the brown dwarfs with ﹩{M}_{2}\sin i\lt 42.5\,{M}_{{\rm{J}}}﹩, while gray squares are larger than this mass. The dashed line indicates the maximum eccentricity for systems unaffected by tides when adopting a circularization period (see Halbwachs et al. 2005) of 10 days. The KOIs are denoted as red squares or triangles, depending on the mass.
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