Astrometric positions of the five largest Uranian satellites from 750 CCD f
rames taken at the oppositions of 1995 through 1998 are presented. The imag
es were obtained over 35 nights. Observed positions are compared with the c
alculated positions from GUST86. The standard deviations are better than 0.
"05 for the four largest satellites and 0."08 for Miranda.