Fig. 3
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One of the images of the occultation obtained from the Astronomical Observatory Cluj-Napoca in Romania (see Table A.1 for details). The source marked as “1” corresponds to the occulted star plus Huya before the beginning of the occultation. The other marked sources were used as reference stars. The FoV of the image is 20 × 13 arcmin, north is up and east is to the left.
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