Fig. 8
Signal-to-noise ratio of synthetic planets measured in the images of HIP 118008 after ADI (solid lines) and ASDI (dashed lines) as a function of mass for several separations. The cut-off at low masses is due to the evolutionary model BT-Settl (see text). The horizontal dotted black line indicates the signal-to-noise ratio used to derive the mass sensitivity limits (see text).
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