\begin{table}%t2
%\centering
\par
\caption{Maximum difference between DE405 and INPOP05 (with the
same initial conditions) in range ($r$), latitude ($\phi$) and
longitude ($\lambda$). If $(x,y,z)$ are the heliocentric (geocentric
for the Moon) coordinates of the planet in the equatorial reference
frame of the ICRF, then $r=\sqrt{(x^2+y^2+z^2)}$, $\phi = \arcsin
(z/r)$ and $\lambda = \arctan(y/x)$. EMB is the Earth-Moon
Barycenter. For the librations of the Moon, $\phi$, $\theta$ and $\psi$ 
are the usual Euler's angles (see Newhall et~al.  \cite{Newhall1983}, Sect.~II.D). 
Comparisons are made over the whole time interval of
DE405 (--400 yr to 200 yr with origin at J2000); Col.~1: from --30 yr
to +30 yr; Col.~2: from --100 yr to +100 yr; Col.~3: from --400 yr to
200 yr.}
\small
\begin{tabular}{rrrr}
 \hline \hline
 \multicolumn{4}{c}{Heliocentric range $r$ (m)} \\
 \hline
 Mercury & 6.2 & 26 & 228 \\
 Venus & 0.5 & 2.1 & 18 \\
 EMB & 1.6 & 7.7 & 60 \\
 Mars &58 &517 &3365 \\
 Jupiter &31 &108 &467 \\
 Saturn &20 &36 &121 \\
 Uranus &38 &45 &69 \\
 Neptune &35 &77 &80 \\
 Pluto &31 &119 &283 \\
 Moon (geocentric) &0.009 &0.034  &0.540 \\
 \hline
 \multicolumn{4}{c}{Longitude $\lambda$ ($\mu$as)} \\
 \hline
 Mercury & 174 &749 &6637 \\
 Venus &78 &534 &6270 \\
 EMB &32 &286 &2494 \\
 Mars &354 &6600 &42070 \\
 Jupiter &57 &276 &1012 \\
 Saturn &16 &51 &201 \\
 Uranus &4 &14 &41 \\
 Neptune &0.7 &14 &39 \\
 Pluto &0.9 &7 &44 \\
 Moon (geocentric) &60 &170 &6173 \\
 \hline
 \multicolumn{4}{c}{Latitude $\phi$ ($\mu$as)} \\
 \hline
 Mercury &65 &268 &2373 \\
 Venus &30 &207 &2262 \\
 EMB &13 &113 &979 \\
 Mars &152 &2602 &16970 \\
 Jupiter &23 &102 &383 \\
 Saturn &5 &17 &67 \\
 Uranus &0.6 &5 &15 \\
 Neptune &0.2 &5 &14 \\
 Pluto &0.4 &3 &19 \\
 Moon (geocentric) &25 &73 &2478 \\
 \hline
\multicolumn{4}{c}{Lunar librations ($\mu$as)} \\
\hline
$\phi$ & 900   &  900  &  1000  \\
$\theta$ & 400   & 400   &  400  \\
$\psi$ & 800  & 800  & 5800   \\
\hline
\end{tabular}
\label{tab1}
\end{table}