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Fig. 4

image

Radial distribution of the detection limits. On the left, blue graphs display contrast as a function of the angular distance in milliarcseconds, this expresses the performance of the detection. On the right, green graphs display estimated mass detection limits (according to the BT-Settl model) as a function of separation in AU. In order to keep track of the azimuthal variation, the lower thick line represents the minimum value found at a given radial distance r, while upper thin line is the maximum value. Black dots represent companion within the known planetary systems.

This figure is made of several images, please see below:

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