I spent most of the second quarter of 1992 with the reduction of the astrometry data. As of end of June, the preliminary reduction of almost all of the data taken since 1988 is completed. Despite lots of problems with many observing sessions, the results are encouraging. In case of good seeing conditions, no technical problems and five observing nights on the N-S and E-S baselines, the formal errors of the derived star positions are about 10 milliarcseconds in right ascension and 5 mas in declination. This empirical result is derived from four sessions in the summer of 88, 89, and 90. (The error in declination is smaller since the N-S baseline is most sensitive to declination offsets and the E-S baseline is not really a match for it with respect to the right ascensions. Also, the N-S baseline was used more often than the E-S baseline). The repeatability of the star positions from session to session appears to be somewhat worse than the formal errors suggest, typically by a factor of 1.5 to 2. A change of the observing lists to two complementary lists in 1991 unfortunately had the effect that as the total time per session did not increase, the amount of data on each list was relatively small. This summer we are therefore planning extensive astrometry sessions on the old and one of the new lists. At the beginning of April, I attended the IAU colloquium on "Complementary Approaches to Double & Multiple Star Research", held at Callaway Gardens near Atlanta, GA. I presented a poster on my own research on observations of spectroscopic binaries with the Mt Wilson interferometer. I spent two weeks on Mt Wilson for observations of binaries. Although the nights were mostly clear, the seeing was bad almost all the time. By reducing the observing list to only one or two program stars with their calibrators, I was able to get useful data, however. A paper on "MERLIN and VLBI observations of the quasar 0836+710: Morphology of parsec-kiloparsec scale jet", radio astronomical research completed during my time in Bonn, was accepted for publication by Astronomy and Astrophysics journal.