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.
@article{arxiv.astro-ph/0303527,
title = {The Torino Observatory Parallax Program: White Dwarf Candidates},
author = {R. L. Smart and M. G. Lattanzi and B. Bucciarelli and G. Massone and R. Casalegno and G. Chiumiento and R. Drimmel and L. Lanteri and F. Marocco and A. Spagna},
journal= {arXiv preprint arXiv:astro-ph/0303527},
year = {2009}
}