\begin{table}%t3
%\centering
\par
\caption{\label{table:test3}Results of the photometric inversion of simulated Eunomia-like shaped asteroids on different asteroidal orbits.}
\begin{tabular}{ccccccccc}
\hline\hline
Simulated & $N$ & \multicolumn{1}{c}{$\lambda$(pole)} &
\multicolumn{1}{c}{$\beta$(pole)} & \multicolumn{1}{c}{Period} &
 $b/a$ & $c/a$ & $k$ & $\epsilon$ \\
Orbit & & \multicolumn{1}{c}{(deg)} & \multicolumn{1}{c}{(deg)} &
\multicolumn{1}{c}{(h)} &   &
  & (mag/$^{\circ}$)  & (mag) \\
\hline 
15  & $85$ & $57.8\pm0.4$ & $72.9\pm0.1$ & $19.150448\pm0.000015$ &
$0.81\pm0.01$ & $0.60\pm0.00$ & $0.022\pm0.000$ & $0.045$ \\
24 (1) & $84$ & $45.8\pm0.1$ & $49.2\pm0.1$ & $19.150410\pm0.000001$
& $0.66\pm0.00$ & $0.59\pm0.00$ & $0.023\pm0.000$ & $0.033$ \\
24 (2) & $84$ & $227.8\pm0.1$ & $49.1\pm0.1$ &
$19.150411\pm0.000002$ & $0.66\pm0.01$ & $0.59\pm0.00$ & $0.023\pm0.000$ & $0.033$ \\
311  & $62$ & $59.5\pm0.3$ & $55.6\pm0.3$ & $19.150247\pm0.000008$ &
$0.70\pm0.00$ & $0.65\pm0.00$ & $0.024\pm0.000$ & $0.038$ \\
319  & $64$ & $46.1\pm0.3$ & $50.4\pm0.1$ & $19.150375\pm0.000009$ &
$0.68\pm0.00$ & $0.64\pm0.00$ & $0.021\pm0.000$ & $0.033$ \\
320  & $48$ & $45.6\pm0.2$ & $43.0\pm0.1$ & $19.150362\pm0.000009$ &
$0.67\pm0.00$ & $0.63\pm0.00$ & $0.024\pm0.000$ & $0.042$ \\
326  & $97$ & $47.2\pm0.2$ & $49.1\pm0.1$ & $19.149561\pm0.000009$ &
$0.69\pm0.00$ & $0.66\pm0.00$ & $0.019\pm0.000$ & $0.040$ \\
363 (1) & $44$ & $248.1\pm0.1$ & $47.9\pm0.3$ &
$19.149723\pm0.000011$ & $0.67\pm0.00$ & $0.67\pm0.00$ & $0.020\pm0.000$ & $0.040$ \\
363 (2) & $44$ & $55.8\pm0.4$ & $51.5\pm0.1$ &
$19.149674\pm0.000013$ & $0.67\pm0.00$ & $0.64\pm0.01$ & $0.022\pm0.010$ & $0.041$ \\
391  & $81$ & $58.5\pm0.3$ & $51.5\pm0.2$ & $19.149986\pm0.000006$ &
$0.71\pm0.00$ & $0.65\pm0.00$ & $0.021\pm0.000$ & $0.057$ \\
433  & $88$ & $59.3\pm0.4$ & $63.7\pm0.2$ & $19.149860\pm0.000003$ &
$0.73\pm0.00$ & $0.60\pm0.00$ & $0.024\pm0.000$ & $0.084$ \\
472 & $62$ & $46.4\pm0.2$ & $48.7\pm0.2$ & $19.150094\pm0.000007$ &
$0.70\pm0.00$ & $0.66\pm0.00$ & $0.024\pm0.000$ & $0.042$ \\
\hline 
\end{tabular}
\begin{list}{}{}
\item[Note:] $N$ is the number of simulated Gaia detections for each case. The spin
parameters adopted to compute the simulated cases are the following:
Pole $= (48.5^\circ, 51.0^\circ)$, Period $= 19.150000$~h.
\end{list}
\end{table}