Fig. 7.
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Colour-magnitude F444W–F277W vs F444W magnitude (top) and colour-colour F444W–F277W vs F200W–F115W diagram (bottom) of the HELM samples. The shaded grey area is the LRD selection criteria by Barro et al. (2024, top) and by Greene et al. (2024, bottom). We show only HELM galaxies with S/N > 3 in the considered filters. The median errors are shown in the top right.
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