Table 2: Parallaxes and proper motions for the six white dwarf candidates in the Torino Program. See text for explanation of columns.
WD Name $N_{\rm s}$ $N_{\rm f}$ $\omega $ mas       $\mu_{\alpha} $ mas/yr    $\mu_{\delta} $ mas/yr    V V-I rms mas $\Delta T$ years

0322-019		 13 83 $59.5 \pm 3.2$ $ 222.5 \pm 1.0$ $-857.5 \pm 1.2$ $16.11 \pm 0.06$ $0.87 \pm 0.11$ 18.07 6.20
0423+120 24 56 $57.6 \pm 2.5$ $-106.7 \pm 1.0$ $-225.5 \pm 0.9$ $15.43 \pm 0.04$ $0.62 \pm 0.05$ 10.94 5.31
1126+185 11 41 $ 0.9 \pm 2.4$ $ 6.0 \pm 1.0$ $ 7.2 \pm 1.1$ $13.97 \pm 0.04$ $0.75 \pm 0.05$ 9.48 6.09
1716+020 21 159 $19.0 \pm 2.3$ $-439.8 \pm 0.7$ $-279.2 \pm 0.9$ $14.30 \pm 0.10$ $0.02 \pm 0.17$ 18.49 6.27
1840-111 77 64 $34.9 \pm 5.1$ $-234.7 \pm 1.6$ $-247.7 \pm 1.5$ $14.18 \pm 0.09$ $0.38 \pm 0.14$ 21.07 6.15
2216+484 130 90 $33.6 \pm 2.5$ $ 146.7 \pm 1.2$ $ -40.3 \pm 0.8$ $16.13 \pm 0.10$ $0.85 \pm 0.15$ 15.19 5.04


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