Fig. 8

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Sensitivity for our direct imaging survey. The isocontours give the number of stars that have the sensitivity to detect companions at a probability of 50% for this given semi-major axis and effective temperature. The dotted lines represent the indicative effective temperatures of the transitions between Y and T-dwarfs (~600 K), T and L-dwarfs (~300 K), L and M-dwarfs (~2000 K).
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