CCD observations of Phoebe in 1998-1999 (Fienga+, 2002)

Physics

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Solar System, Planets, Positional Data

Scientific paper

Topocentric ICRF J2000 Phoebe positions reduced from CCD observations realised with the 1.2m of the OHP Observatory. The positions proposed in the following table is corrected from a systematic effect introduced by the USNO A2.0 reference stars. This correction was estimated after ICRF optical counterparts observations (Fienga and Andrei, 2002, A&A, submitted) (1 data file).

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