Fig. 11.
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Proper motion of a candidate UCD. The postage stamp cutouts show the source in VISTA J, JE, and F115W from JWST. The cutouts are 5″ × 5″ and saturate at 2σ and 5σ below and above the noise level. The red crosshair is placed at the centroid of the source as determined from the VISTA image to highlight the proper motion when observed with Euclid and JWST.
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