\begin{table}%t6
%\centering
\par
\caption{INPOP06 (Col.~5) residuals for each type of observation. Column~3 gives the observational time interval and Col.~4 the number of observations $N$ used in the fit and in the residual computations.  For optical observations, the residuals are given respectively in right ascension and declination ($\alpha$; $\delta$). The  uncertainties are at 1-sigma.}
\begin{tabular}{l l l r c c }
\hline\hline
Planet&
 Type of data & Time interval & $N$ &
 %DE414 & &
 INPOP06 &\\
 & & & & $\langle{(o-c)}\rangle$ & $\sigma$ \\
\hline
Mercury &
Radar [m]&
1971--1998& 444&
%-596.0 & 956 &
--239 & 855 \\
Venus&
Radar [m]&
1964--1990& 737&
--1727 & 4051 \\
& & after 1965 & 488 & 583 & 1385 \\
&
Spacecraft VLBI [mas]&
1990--1994 & 18&
%1.7 & 2.5 &
1.7 & 2 \\
Mars&
Vkg lander radar [m]&
1976--1983 & 1256&
%-5.7 & 18 &
--23 & 18 \\
&
MGS/Odyssey radar [m]&
1999--2005.45 & 10474&
%7.4 & 4.1 &
4.0 & 5.5 \\
&
Vkg Doppler [mm/s]&
1976--1979 & 1501&
%-0.26& 4.5 &
--0.26 & 4.4 \\
&
Pathfinder Doppler [mm/s]&
1997 & 1519&
%-0.34 & 0.97 &
--0.34 & 0.97 \\
&
Spacecraft VLBI [mas]&
1989--2003 & 44&
%0.04 & 0.5 &
0.4 & 0.5 \\
Jupiter&
Spacecraft VLBI [mas]&
1996--1998& 24&
%-1 & 12 &
--9 & 12 \\
&
optical ($\alpha$, $\delta$) [mas] &
1914--2004 & 5536&
%( 4; -24 )& ( 340;332 ) &
(--17; -- 24) & (341 ; 331)\\
Saturn&
 optical ($\alpha$, $\delta$) [mas] &
1914-2004 & 5573&
%(51 ;-7)& ( 342;312 )&
(--6; 13)& (347 ; 311)\\
Uranus&
 optical ($\alpha$, $\delta$) [mas] &
1914--2004 & 3848&
%( 11 ; 13)& (440 ; 370)&
(12; 10) & (357; 366)\\
Neptune&
 optical ($\alpha$, $\delta$) [mas] &
1914--2004 &3898&
%( 12 ; 11)& (404 ; 438)&
(11; 12) & (368; 356)\\
Pluto&
optical ($\alpha$, $\delta$) [mas] &
1989--2004 & 1024&
%(13  ; -0.8)& (264 ; 252)&
(11; --8) & (260; 190)\\
\hline
\end{tabular}
\label{omcINPOP06}
\end{table}