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Fig. 7


Mean probability of detection of our survey as a function of semimajor axis and planet mass (left) and for specific masses, given above or below each curve in MJup, as a function of semimajor axis (right). The mean probability of detection is obtained by averaging the completeness maps of all targets of the survey. β Pic b (orange square) and the 4 planets of the HR 8799 system (red circles) have been overlaid for reference using the current best estimates of their mass and separation. Note that the HR 8799 planets are represented at their projected physical separation because the true physical separation is not yet known precisely.

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