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Fig. 11

image

Recombined images obtained with K-Stacker, when searching for additional companions around β Pictoris and HD 95086, two systems observed in the SHINE survey. At each epoch, the images are rotated and shifted to put the detection on its periastron position found by K-Stacker, and the frames are co-added. In each case, a bright spot can be seen near the coronagraphic mask (red arrow), which corresponds to the best solution found by the algorithm. In the case of β Pic, the corresponding (S/N)KS is 4.8. For HD 95086, the (S/N)KS is 4.4.

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