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Fig. 6.
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mF606W versus mF606W − mF150W2 (panel a) and mF606W versus mF814W − mF150W2 (panel b) CMDs of our selected sample of sources, focusing on the WD CS. The orange error bars on the left side of each panel indicate the photometric uncertainties in colour, derived from ASs, as a function of the mF606W magnitude.
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