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Fig. 2

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Location of the objects shortlisted as candidate UCDs via astrometric selection, for an example 20 × 20 deg2 region, in a colour-magnitude (left) and a reduced proper motion (right) diagram built using Gaia EDR3 sources with parallaxes larger than 10 mas (dark blue dots). The vertical and horizontal red lines mark the boundaries for a source to be shortlisted as candidate UCD. Sources fulfilling these conditions are overplotted in yellow.

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