Top left: parallaxes of Hyades WD candidates as a function of Gaia magnitude. Top right: vector point diagrams for Hyades WD candidates. Bottom left: (G_BP − G,G − G_RP) colour–colour magnitude of all candidates in our 30 pc sample. Bottom right: (G_BP − G_RP,G_RP) colour–magnitude magnitude for our 30 pc sample. The classical WDs from von Hippel (1998) are shown as black dots. The candidates from Schilbach & Röser (2012) are highlighted with their ID number. The Hyades single and binary WDs from Gaia Collaboration (2018a) are depicted as red and blue circles, respectively.