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Fig. 11


Sample-averaged companion exclusion limits (solid line) as a function of orbital period (bottom label) and relative primary-secondary separation (top label, computed for a 5 MJ companion around a 0.08 M primary). The minimum companion mass incompatible with the measurements is shown, i.e. companions on and above the curve are excluded by the data. To illustrate the variation across the sample, we divided it into two groups of targets with lower (9 objets, dashed line) and higher (9 objects, dash-dotted line) exclusion limits. The two tight binaries were excluded.

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