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Fig. 7

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Extinction-corrected Gaia CMD of single WDs and WD+MS candidates from our classification. The ELM region is marked with dotted red lines. ELM WD candidates are shown with filled cyan circles. The remaining single WDs and WD+MS candidates are shown with filled orange and red circles, respectively. The WD cooling models for different masses from Bédard et al. (2020) are also overlaid. The numbers on the cooling track denote their corresponding masses in M.

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