\begin{table}%t4
%\centering
\par
\caption{\label{table:test4}Results of the photometric inversion of simulated Golevka-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  & $85$ & $41.8\pm0.2$ & $54.7\pm0.3$ & $19.149624\pm0.000004$ &
$0.66\pm0.00$ & $0.64\pm0.00$ & $0.027\pm0.000$ & $0.044$ \\
24 (1) & $84$ & $229.6\pm0.2$ & $49.2\pm0.1$ &
$19.150124\pm0.000002$ & $0.61\pm0.00$ & $0.61\pm0.00$ & $0.026\pm0.000$ & $0.041$ \\
24 (2) & $84$ & $47.9\pm0.1$ & $49.3\pm0.1$ & $19.150115\pm0.000001$
& $0.61\pm0.00$ & $0.61\pm0.00$ & $0.026\pm0.000$ & $0.042$ \\
311  & $62$ & $46.0\pm0.5$ & $53.8\pm0.2$ & $19.150163\pm0.000003$ &
$0.63\pm0.00$ & $0.60\pm0.00$ & $0.029\pm0.000$ & $0.045$ \\
319  & $64$ & $45.8\pm0.2$ & $49.2\pm0.1$ & $19.150106\pm0.000003$ &
$0.64\pm0.00$ & $0.64\pm0.00$ & $0.026\pm0.000$ & $0.040$ \\
320  & $48$ & $44.0\pm0.1$ & $46.8\pm0.1$ & $19.150330\pm0.000009$ &
$0.63\pm0.00$ & $0.63\pm0.00$ & $0.024\pm0.000$ & $0.045$ \\
326  & $97$ & $43.5\pm0.2$ & $51.6\pm0.2$ & $19.149358\pm0.000006$ &
$0.65\pm0.00$ & $0.65\pm0.00$ & $0.018\pm0.000$ & $0.056$ \\
363  & $44$ & $47.0\pm0.8$ & $53.3\pm0.5$ & $19.149573\pm0.000008$ &
$0.65\pm0.00$ & $0.62\pm0.01$ & $0.024\pm0.000$ & $0.045$ \\
391  & $81$ & $62.1\pm0.2$ & $51.6\pm0.1$ & $19.149814\pm0.000003$ &
$0.64\pm0.00$ & $0.64\pm0.00$ & $0.021\pm0.000$ & $0.044$ \\
433  & $88$ & $57.1\pm0.0$ & $52.5\pm0.0$ & $19.149919\pm0.000001$ &
$0.64\pm0.00$ & $0.64\pm0.00$ & $0.024\pm0.000$ & $0.101$ \\
472  & $62$ & $46.2\pm0.0$ & $45.7\pm0.0$ & $19.150169\pm0.000002$ &
$0.63\pm0.00$ & $0.63\pm0.00$ & $0.023\pm0.000$ & $0.047$ \\
\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}