Fig. 5

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IFS images of →2 Sco obtained with ASDI-PCA with 25 modes (left panel: first epoch; right panel: second epoch). The star is at the center of the image but not visible due to the presence of the coronagraphic mask – which artificially masks the innermost ~90 mas of the image – and the aggressive data analysis method used. The probable companion CC0 is the source inside the white circle. A background source is visible on the lower left of the first-epoch image.
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