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Fig. 6

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Lucky Camera image of WASP-67. The image size is 45 × 45 arcsec2 and is shown in a logarithmic flux scale with north up and east to the left. The FWHM of the image is . The triangular PSF comes from the telescope in very good seeing. The extra flux north-west of WASP-67 A is not a real contaminating flux source but an optical ghost from the star caused by internal reflections within the beamsplitters.

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