\begin{table}%t5
%\centering
\par
\caption{\label{table:test5}Results of the photometric inversion of simulated Eros-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  & $85$ & $59.8\pm0.3$ & $54.0\pm0.7$ & $19.150029\pm0.000024$ &
$0.24\pm0.02$ & $0.22\pm0.01$ & $0.018\pm0.001$ & $0.054$ \\
24  & $84$ & $45.5\pm0.1$ & $44.1\pm0.2$ & $19.150292\pm0.000002$
& $0.28\pm0.01$ & $0.28\pm0.01$ & $0.022\pm0.001$ & $0.058$ \\
311 & $62$ & $50.4\pm0.2$ & $53.0\pm0.1$ & $19.150183\pm0.000005$
& $0.41\pm0.00$ & $0.41\pm0.00$ & $0.026\pm0.000$ & $0.091$ \\
319 & $64$ & $50.5\pm0.6$ & $47.2\pm0.2$ & $19.150310\pm0.000013$
& $0.42\pm0.01$ & $0.42\pm0.01$ & $0.021\pm0.000$ & $0.060$ \\
320 & $48$ & $43.4\pm0.9$ & $42.7\pm1.4$ & $19.150424\pm0.000021$
& $0.34\pm0.03$ & $0.34\pm0.03$ & $0.024\pm0.001$ & $0.068$ \\
326 & $97$ & $49.3\pm0.4$ & $50.4\pm0.7$ & $19.149266\pm0.000012$
& $0.40\pm0.01$ & $0.40\pm0.01$ & $0.025\pm0.000$ & $0.058$ \\
363 & $44$ & $45.1\pm0.4$ & $54.0\pm0.3$ & $19.149646\pm0.000037$
& $0.41\pm0.00$ & $0.41\pm0.00$ & $0.021\pm0.001$ & $0.073$ \\
391 & $81$ & $55.2\pm0.8$ & $51.4\pm0.2$ & $19.150162\pm0.000021$
& $0.47\pm0.00$ & $0.44\pm0.00$ & $0.022\pm0.000$ & $0.077$ \\
433 & $88$ & $49.0\pm0.2$ & $53.4\pm0.3$ & $19.149835\pm0.000006$
& $0.43\pm0.00$ & $0.40\pm0.00$ & $0.024\pm0.000$ & $0.143$ \\
472 & $62$ & $44.7\pm0.5$ & $52.0\pm0.3$ & $19.149876\pm0.000008$
& $0.43\pm0.00$ & $0.43\pm0.00$ & $0.023\pm0.000$ & $0.081$ \\
\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: Pole $=(48.5^\circ, 51.0^\circ)$, Period $= 19.150000$~h.
\end{list}
\end{table}