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6 Comparison with Taylor (1998)

The rms's, and means are given in arcseconds in Table 6 where S.E.M. is the standard error of the mean, $N_{\rm u}$is the number of observations used and $N_{\rm r}$ is the number of observations rejected. 11 outliers with residuals $\gt 0\hbox{$.\!\!^{\prime\prime}$}15$ were rejected out of 1028 measures.
  
Table 6: Comparison with the numerical integration of Taylor (1998)

\begin{tabular}
{llrlrr}
\hline\noalign{\smallskip}
Satellite & Rms & Mean & S.E...
 ...prime\prime}$}0024$\space & 125 & 2 \\ \noalign{\smallskip} 
\hline\end{tabular}

In deriving these figures no change was made to the initial conditions of Taylor (1998). These values are comparable to the photographic observations of Veiga & Vieira Martins (1995a) but smaller than the CCD observations of Veiga & Vieira Martins (1995b). The significance of these differences should not be stressed because Veiga and Vieira Martins compared their observations to Laskar & Jacobson (1987) where we compared with Taylor (1998).


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