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Astrometric positions of the ve largest Uranian satellites from 750 CCD frames taken at the oppositions of 1995 through 1998 are presented. The im- ages were obtained over 35 nights. Observed positions are compared with the calculated positions from GUST86. The standard deviations are better than 0: 00 05 for the four largest satellites and 0: 00 08 for Miranda.

CCD astrometric observations of Uranian satellites: 1995-1998