We have calculated the root-mean-square residuals of the observations in the form of inter-satellite and measures. In Table 5 we present the statistics for Tethys, Dione, Rhea and Titan. The rejection level was . For comparison, we give the same statistics for the observations published in Harper et al. (1997). The orbital models are those of Harper & Taylor (1993).
Copyright The European Southern Observatory (ESO)