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Fig. 11

image

Third-body mass allowed by the RV drift for a given period assuming circular orbits for KOI-206 (left) and KOI-680 (right). The median of the distribution is represented by a solid line, and the 1, 2, and 3σ confidence intervals are represented with three different gray levels. The dotted lines separate the planetary, brown dwarf, and star regimes.

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