the sky ($\delta > -23\deg $). Part I of the NPM program (“NPM1”), outside the disk of the Milky Way ($|b| > 10$ deg), was completed in 1993; the Lick NPM1 Catalog (Klemola, Hanson, and Jones 1993) contains 148,940 stars, with proper motions accurate to 5 mas/yr, and positions accurate to 02 or better. Part II of the NPM program (“NPM2”), in the Milky Way sky, will be completed in roughly three years.

We searched for program stars within a $\pm 10\arcsec \times 10\arcsec $ error box, centered on the NPM1 catalog positions (updated to epoch 2000.0 using the NPM1 proper motions). This procedure found matches for 241 stars; 95 % of these comprise a tight core with RMS position difference 05 in each coordinate, and can be considered unambiguous matches. The remaining 5 % can be considered highly probable matches; agreement between the cataloged and NPM1 apparent magnitudes (better than $\pm \sim 1$ mag) confirms these.

NPM1 proper motions for an additional 58 RR Lyrae stars, from the list of Layden et al. (1996), were added to our catalogue, making a total of 299 stars with NPM1 proper motion data.

### The STARNET Catalog

The proper motions of the 