\begin{table}%T3
 \caption{\label{newmass}Asteroid GMs fitted in INPOP08. }
 \small%\centerline
{
 \begin{tabular}{l l r l l l l}
 \hline
 \hline 
 Asteroid & INPOP08 &  Others  & $r$ & Type & $\rho$ & \\
& $10^{-11}~M_{\odot}$ &  $10^{-11}~M_{\odot}$ & km & & g~cm$^{-3}$ & [m]\\
 \hline 
%3 Juno & 0.753 $\pm$ 0.02 & 1.49 $\pm$ 0.15 [1] & 117 $\pm$ 6 & S & 2.29 $\pm$ 0.3& 184\\
%&& 1.49 $\pm$ 0.15 [1]& & &&\\
%&& 1.54  [4]& & &&\\
 16 Psyche & 1.596 $\pm$ 0.032 & 1.29 $\pm$ 0.17 [1] & 126.6 $\pm$ 2.0 & M & 3.7 $\pm$ 0.1 & 138\\
&& 1.688 [4]& & &&\\
 29 Amphitrite &0.491 $\pm$ 0.09 & 1.00 $\pm$ 0.35 [1] & 106.1 $\pm$ 3.4 & S & 1.9 $\pm$ 0.4 & 118\\
&& 0.684 [4]& & &&\\
 14 Irene & 0.071 $\pm$ 0.01 & 0.2623 [2] & 76.0 $\pm$ 8.0 & S & 0.8 $\pm$ 0.3 & 69\\
& & 0.413 $\pm$ 0.073 [3] & & &&\\
&& 0.263 [4]& & &&\\
704 Interamnia & 1.623 $\pm$ 0.01 &  3.58 $\pm$ 0.42 [1] & 158.3 $\pm$ 2.0  & C & 1.9 $\pm$ 0.1& 65\\
&& 1.862 [4]& & & &\\
532 Herculina & 0.546 $\pm$ 0.01 & 0.667 [2] & 111.2 $\pm$ 2.0 & S & 1.9 $\pm$ 0.1& 63\\
&& 0.669[4]& & &&\\
 6 Hebe & 0.016 $\pm$ 0.011 & 0.759 $\pm$ 0.142 [1] & 92.5 $\pm$ 1.5 & S & 0.1 $\pm$ 0.1 & 63\\
 & & 0.255 [2] & & &&\\
&& 0.457 [4]& & &&\\
 52 Europa & 1.724 $\pm$ 0.100 & 0.976 $\pm$ 0.22 [1] & 151.25 $\pm$ 2.7 & C & 2.4 $\pm$ 0.2& 52\\
&& 1.023 [4]& & &&\\
9 Metis & 0.115 $\pm$ 0.100 & 1.03 $\pm$ 0.24 [1] & 95.0 $\pm$ 9.5 & S & 0.6 $\pm$ 0.5 & 49\\
 & & 0.600 [2] & & &&\\
&& 0.428 [4]& & &&\\
 19 Fortuna  & 0.202 $\pm$ 0.02 & 0.541 $\pm$ 0.008 [1] & 101.7  & C& 0.9 $\pm$ 0.1& 48\\
&& 0.350 [4]& & &&\\
128 Nemesis &0.169 $\pm$ 0.033 & &94.1 $\pm$ 2.0 & C & 1.0 $\pm$ 0.2 & 42\\
18 Melpomene & 0.091 $\pm$ 0.02 & 0.151 $\pm$ 0.051 [3] & 70.3 $\pm$ 1.5 & S & 1.2 $\pm$ 0.3& 40\\
&& 0.201 [4]& & &&\\
 15 Eunomia & 2.230 $\pm$ 0.018 & 1.68 $\pm$ 0.08 [1] & 127.7 $\pm$ 7.0 & S & 5.0 $\pm$ 0.7& 37\\
&& 1.239 [4]& & &&\\
88 Thisbe &0.863 $\pm$ 0.026 & 0.57 $\pm$ 0.18 [1] & 116.0 $\pm$ & C & 2.6 $\pm$ 0.1& 36\\
409 Aspasia  & 0.105 $\pm$ 0.003 &0.163 [4] &80.8 $\pm$ 4.0& C & 0.9 $\pm$ 0.1& 29\\
 216 Kleopatra & 0.353  $\pm$ 0.012 & 0.255 [2]&67.5 $\pm$  & M & 5.3 $\pm$ 0.2 & 27\\
&& 0.226 [4]& & &&\\
21 Lutetia & 0.1034 $\pm$ 0.03 & 0.129 $\pm$ 0.012 [3]& 47.9 $\pm$ 4.1 & M& 4.4 $\pm$ 1.3&24\\
&& 0.105 [4]& & &&\\
 31 Euphrosyne & 2.99 $\pm$ 0.68 & 1.54 [2] & 127.95 $\pm$ 5.5 & C & 6.7 $\pm$ 1.6& 23\\
& & 0.313 $\pm$ 0.059 [3] & & &&\\
&& 0.860 [4]& & &&\\
23 Thalia & 0.003 $\pm$ 0.001& &53.8 $\pm$ 2.2 & S & 1.06 $\pm$ 0.08& 23\\
&& 0.097 [4]& & &&\\
354 Eleonora & 0.488 $\pm$ 0.035 & 0.246  [2] &77.6 $\pm$ 4.2 & S & 4.9 $\pm$ 0.4& 22\\
&& 0.247 [4]& & &&\\
 192 Nausikaa & 0.137 $\pm$ 0.041 & 0.081 [4]& 51.6 $\pm$ 1.0 & S & 4.6 $\pm$ 1.4& 22\\
747 Winchester & 0.0004 $\pm$ 0.0002 & 0.148[4] &85.9 $\pm$ 1.5 & C & 3e-3 $\pm$ 1e-3 & 22\\
129 Antigone& 0.717 $\pm$ 0.014& &104.58 $\pm$ & M & 3.0 $\pm$ 0.1& 21\\
41 Daphne & 0.527 $\pm$ 0.05& 0.467 [2] & 87.00 $\pm$ 6.0 & C & 3.8 $\pm$ 0.7& 20\\
&&0.398[4]& & &&\\
173 Ino& 0.366 $\pm$  0.030 &&77.0 $\pm$ 1.6 & C & 3.8 $\pm$ 0.3& 20\\
89 Julia &0.359 $\pm$ 0.014& & 75.8 $\pm$ 1.5 & C & 4.0 $\pm$ 0.4& 15\\
 %3 Juno &  &  [2]   \\
8 Flora & 0.535 $\pm$ 0.005 & 0.178 [2] & 67.9 $\pm$ 1.0 & S & 8.1 $\pm$ 0.5 & 14\\
& & 0.426 $\pm$ 0.045 [3]& & &&\\
&& 0.178 [4]& & &&\\
  12 Victoria & 0.117 $\pm$ 0.003& &56.4 $\pm$ 1.5 & S & 3.1 $\pm$ 0.2& 13\\
 139 Juewa& 0.359 $\pm$  0.010 &0.142[4]&78.3 $\pm$ 1.5 & C  & 3.6 $\pm$ 0.10& 10\\
 \hline
 \end{tabular}}
 \smallskip
 Other values deduced from planetary ephemerides
 are presented for comparison. Reference [1] is for Baer \& Chelsey (\cite{Baer2008}); [2] are values estimated in DE414 but not published with errorbars. They are directly extracted from the DE414 header; [3]~is for Baer et~al. (\cite{Baer2008e}) and [4]~for DE421 values as published by Folkner et~al. (\cite{Folkner2008}). The given uncertainties are  formal accuracy given at 1-sigma. Columns~4 and~5 are the physical characteristics of the objects: Col.~4 is the radius in kilometers, and spectral type is given in Col.~5. In Col.~6 we give the densities obtained using the given radius and the estimated masses  in Col.~2. Density errorbars are estimated with the given mass 1-sigma uncertainties and accuracies on radius  provided by the PDS website. The last column gives the maximum impact of each asteroid on the Earth-Mars distances over the 1998 to~2008 interval.
    \vspace*{0.5mm}
    \end{table}