Kinematic absolute magnitude versus color diagrams for Hyades white dwarf candidates (filled circles) and probable non-Hyades members (open circles) identified in Paper II. Binaries are marked as filled triangles and by their numbers from Table 1, although in most cases, they are too bright for the range of absolute magnitudes shown in the figure. Theoretical cooling sequences are shown from log g = 7.0 (dotted line) to log g = 9.0 (solid line) in steps of 0.5 dex.