We have calculated the root-mean-square residuals of the observations in the form
of inter-satellite 
and
measures. The orbital models are those of Harper
& Taylor (1993, 1994). In Table 10 we present the statistics for Tethys, Dione, Rhea and
Titan. The rejection level was 
and this table is
directly comparable with Table 3b in Harper & Taylor
(1994). For comparison, we give the same statistics for
the top
five datasets listed in that paper.
Table 10: Statistics of observed-minus-computed residuals for observations
of Tethys, Dione, Rhea and Titan. Type code ``C 1'' denotes 
and 
measures from CCD images. 
is the number of observations included in the solution. 
is the total number of
observations in the dataset. 
is the mean residual and 
is the standard deviation
about the mean. See Strugnell & Taylor (1990)