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Fig. 1.

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PSF-corrected FWHM size as a function of IE magnitude for sources in the NGC 2403 field. Previously known GCs are shown with red filled circles while the new candidates identified in H25 are shown with open circles. Data for Milky Way GCs are also included, scaled to the distance of NGC 2403 (black filled circles). The red line indicates our size cut for the selection of cluster candidates.

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