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Fig. 1

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Combined two-epoch NIRC2 image of Vega in the Ms band using ADI with 10% of the KLIP components for demonstration purposes. We did not identify point sources that were more than 5σ levels beyond the noise of a similar angular separation from the star. The pixel values correspond to lower limits of contrast values due to over- and self-subtraction with KLIP and ADI, respectively.

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