Table 5: Standard deviation of U, V, W for the 361 SPY thin-disk white dwarfs, $\sigma _{U}$ , $\sigma _{V}$ , and $\sigma _{W}$ from Soubiran et al. (2003) are shown for comparison.
$\sigma _{U}$ $\sigma _{V}$ $\sigma _{W}$

${\rm km~s^{-1}}$ ${\rm km~s^{-1}}$ ${\rm km~s^{-1}}$

Thin-disk WDs

(our sample) 34 24 18

Thin-disk stars

(Soubiran et al.) 39 20 20

**Table 5:** Standard deviation of U, V, W for the 361 SPY thin-disk white dwarfs, $\sigma _{U}$ , $\sigma _{V}$ , and $\sigma _{W}$ from Soubiran et al. (2003) are shown for comparison.
	$\sigma _{U}$	$\sigma _{V}$	$\sigma _{W}$
	${\rm km~s^{-1}}$	${\rm km~s^{-1}}$	${\rm km~s^{-1}}$
Thin-disk WDs
(our sample)	34	24	18
Thin-disk stars
(Soubiran et al.)	39	20	20

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