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Fig. 2.

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Simulated images of GCs added to the Euclid VIS image of NGC 2403, next to the clusters D6 (top), JC15 (centre), and a new candidate closer to the centre of NGC 2403 (bottom). In each panel, simulated GCs are shown for masses of 105M, 3 × 105M, and 106M (left to right) a half-light radius of 3 pc, and an assumed age of 10 Gyr. Each panel measures 295 × 70 VIS pixels ( 29 . 5 × 7 . 0 $ 29{{\overset{\prime\prime}{.}}}5\times7{{\overset{\prime\prime}{.}}}0 $).

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