Fig. 10
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Euclid VIS-NISP colours as a function of IE measured using aperture photometry within 1 Re of the 1100 dwarf galaxy candidates and the bright galaxy sample in the ERO Perseus field from Cuillandre et al. (2025b) shown in violet and light grey, respectively. The magnitudes were corrected for extinction before the colours were computed, as described in Sect. 5.1.
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