Table 7: Standard deviation of U, V, W for the seven SPY halo white dwarfs, $V_{\rm lag}$ , $\sigma _{U}$ , $\sigma _{V}$ , and $\sigma _{W}$ from Chiba & Beers (2000) shown for comparison.
$\sigma _{U}$ $\sigma _{V}$ $\sigma _{W}$

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

Halo white dwarfs

(our sample) 138 95 47

Halo stars

(Chiba & Beers) 141 106 94

**Table 7:** Standard deviation of U, V, W for the seven SPY halo white dwarfs, $V_{\rm lag}$ , $\sigma _{U}$ , $\sigma _{V}$ , and $\sigma _{W}$ from Chiba & Beers (2000) shown for comparison.
	$\sigma _{U}$	$\sigma _{V}$	$\sigma _{W}$
	${\rm km~s^{-1}}$	${\rm km~s^{-1}}$	${\rm km~s^{-1}}$
Halo white dwarfs
(our sample)	138	95	47
Halo stars
(Chiba & Beers)	141	106	94

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