  We present astrometric results on two millisecond pulsars, PSR B1257+12 and
PSR J1022+1001, as carried out through VLBI. For PSR B1257+12, a
model-independent distance of $710_{\rm -38}^{\rm +43}$ pc and proper motion of
($\mu_{\rm \alpha}=46.44\pm0.08$ mas/yr, $\mu_{\rm \delta}=-84.87\pm0.32$
mas/yr) were obtained from 5 epochs of VLBA and 4 epochs of EVN observations,
spanning about 2 years. The two dimensional proper motion of PSR J1022+1001
($\mu_{\rm \alpha} \sim -10.13$ mas/yr, $\mu_{\delta} \sim 16.89$ mas/yr) was
also estimated, using 3 epochs of EVN observations. Based on our results, the
X-ray efficiency of PSR B1257+12 should be in the same range as other
millisecond pulsars, and not as low as previously thought.
