\begin{table}%t2
 \caption{\label{paramphy}Physical parameters fitted in INPOP08.  }
 \small%\centerline
{
 \begin{tabular}{l l l r r r l} 
 \hline\hline 
 &Unit& 
 DE414&
 DE421&
EPM 2008 & 
 INPOP06 & INPOP08
 \\
 \hline \noalign{\smallskip}
 Mass of Ceres &
 $10^{-10}~M_{\odot}$& 
 4.699 $\pm$ 0.028&
 4.685 &
4.712 $\pm$ 0.006 &
 4.756 $\pm$ 0.020&
 4.658 $\pm$ 0.045\\
 Mass of Vesta&
 $10^{-10}~M_{\odot}$& 
 1.358 $\pm$ 0.016 &
 1.328  &
 1.344 $\pm$ 0.003&
 1.348 $\pm$ 0.015 &
 1.392 $\pm$ 0.015 \\
 Mass of Pallas&
 $10^{-10}~M_{\odot}$& 
 1.026 $\pm$ 0.028&
 1.010  &
1.027 $\pm$ 0.007 &
 1.025 $\pm$ 0.005 &
 1.076 $\pm$  0.010\\
 Mass of Juno&
 $10^{-10}~M_{\odot}$& 
 0.149 $\pm$ 0.015&
 0.116  &
n/a &
 NE &
 0.075 $\pm$ 0.015 \\
 Mass of Iris&
 $10^{-10}~M_{\odot}$& 
 0.060 $\pm$ 0.010 &
 0.060 &
n/a &
 0.058 $\pm$ 0.005 &
 0.050 $\pm$  0.010\\
 Mass of Bamberga&
 $10^{-10}~M_{\odot}$& 
 0.047 $\pm$ 0.007&
 0.048 &
n/a &
 0.046 $\pm$ 0.003 &
 0.056 $\pm$   0.004\\
 Mass of Ring&
 $10^{-10}~M_{\odot}$& 
 0.30 & NE &n/a &
 0.34 $\pm$ 0.1& 1.0 $\pm$ 0.3\\
 Distance of Ring&
 UA& 
 2.8 &  NE & 
n/a &
 2.8  & 3.14 \\
 Density of the C class&
 & 
 1.62 $\pm$ 0.07&
 1.09  &
n/a &
 1.56 $\pm$ 0.02 &
 1.54 $\pm$ 0.07 \\
 Density of the S class&
 & 
 2.08 $\pm$ 0.19&
 3.45&
n/a &
 2.18 $\pm$ 0.04 &
 1.94 $\pm$ 0.14\\
 Density of the M class&
 & 
 4.32 $\pm$ 0.37 &
 4.22  &
n/a &
 4.26 $\pm$ 0.12 &
 4.98 $\pm$ 0.50\\
 Sun J2&
 $10^{-7}$& 
 2.34 $\pm$ 0.49 &
 2.0 &
n/a &
 2.46 $\pm$ 0.40 &
 1.82 $\pm$ 0.47  \\
 EMRAT &
 & 81.300568 & 81.300569 & 81.3005690 $\pm$ 0.0000001 & NE & 81.300540 $\pm$ 0.00005\\
 AU-${\rm AU_{IERS03}}$ & m & 9.8 $\pm$ 0.15 & 8.6 $\pm$ 0.15 & 4.4 $\pm$ 0.10 & NE &  8.22 $\pm$ 0.11 \\ 
 \hline
 \end{tabular}}
 \smallskip
 Other values deduced from planetary ephemerides
 are presented for comparison. EPM08 stands for Pitjeva (\cite{Pitjeva2008}). The uncertainties are given at 5-sigma for the GMs and 1 formal sigma for others. n/a stands for non-avalaible and NE as non-estimated. For~AU, the presented values are the differences in meters between the fitted values and the AU value of the IERS conventions 2003, ${\rm AU_{IERS03}} = 14~9597~870.691$~km.
  \vspace*{2mm}
  \end{table}