  We present a Catalog of high proper motion (HPM) stars detected in the
foreground of central parts of the Magellanic Clouds. The Catalog contains 2161
objects in the 4.5 square degree area towards the LMC, and 892 HPM stars in the
2.4 square degree area towards the SMC. The Catalog is based on observations
collected during four years of the OGLE-II microlensing survey. The Difference
Image Analysis (DIA) of the images provided candidate HPM stars with proper
motion as small as 4 mas/yr. These appeared as pseudo-variables, and were all
measured astrometrically on all CCD images, providing typically about 400 data
points per star. The reference frame was defined by the majority of background
stars, most of them members of the Magellanic Clouds. The reflex motion due to
solar velocity with respect to the local standards of rest is clearly seen. The
largest proper motion in our sample is 363 mas/yr. Parallaxes were measured
with errors smaller than 20% for several stars.
