  We present parallax determinations for six white dwarf candidates in the
Torino Observatory Parallax Program. The absolute parallaxes are found with
precisions at the 2-3 milliarcsecond level. For WD 1126+185 we find a distance
incompatible with being a white dwarf, implying an incorrect classification.
For WD 2216+484 we find our distance is consistent with a simple DA white dwarf
rather than a composite system as previously proposed in the literature. In
general it is found that the published photometric distance is an overestimate
of the distance found here.
