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Fig. 8


Expected photometric errors for different contrasts as a function of separation from the central star. Results obtained with KLIP (red line) and SD (blue line) are compared. Each point represents the median of the errorbar on the 39 IFS channels. Only detected planets are considered in this analysis. Very few planets with contrast of 10-5 are detected, as shown in Table 3, so the corresponding plot is not shown.

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

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