\begin{table}%t2
\par
\caption {Physical properties of the sample inferred from their SED.
\label{tab_phys}}
%\centerline
 {\begin{tabular}{lccccccc}
\hline\hline                 % inserts double horizontal lines
Name & $\log M_*$ (BC03) & $\log M_*$ (M05) & $M_B$ & $U-V$ & SFR & 
  $E(B-V)$$_*$  & Age \\
     & $[M_{\odot}]$    & $[M_{\odot}]$   & [mag]     & [mag]& 
     $[M_{\odot}~\rm  yr^{-1}]$
 & [mag]   & [Gyr] \\
\hline
CDFa-C9 & 10.18$\rm ^{+0.40}_{-0.08}$ &10.13$\rm ^{+0.30}_{-0.05}$ &--22.36 & --0.24 & 265 & 0.25$\rm ^{+0.05}_{-0.10}$ &0.06$\rm ^{+0.25}_{-0.01}$ \\
CDFS-4414 & 10.57$\rm ^{+0.19}_{-0.22}$ &10.48$\rm ^{+0.06}_{-0.23}$ &--22.47 & --0.02 & 113 & 0.20$\rm ^{+0.05}_{-0.10}$ &0.39$\rm ^{+0.60}_{-0.29}$ \\
CDFS-4417 & 10.29$\rm ^{+0.37}_{-0.11}$ &10.32$\rm ^{+0.29}_{-0.10}$ &--22.79 & --0.35 & 438 & 0.25$\rm ^{+0.05}_{-0.10}$ &0.05$\rm ^{+0.23}_{-9.99}$ \\
CDFS-6664 & 9.49$\rm ^{+0.10}_{-0.23}$ &9.30$\rm ^{+0.22}_{-0.08}$ &--20.93 & --0.70 & 35 & 0.10$\rm ^{+0.10}_{-0.04}$ &0.10$\rm ^{+0.09}_{-0.05}$ \\
CDFS-16767 & 10.05$\rm ^{+0.10}_{-0.16}$ &9.90$\rm ^{+0.13}_{-0.13}$ &--21.90 & --0.49 & 84 & 0.15$\rm ^{+0.05}_{-0.05}$ &0.12$\rm ^{+0.07}_{-0.07}$ \\
CDFS-11991 & 9.69$\rm ^{+0.12}_{-0.15}$ &9.64$\rm ^{+0.18}_{-0.08}$ &--21.64 & --0.46 & 55 & 0.10$\rm ^{+0.05}_{-0.04}$ &0.10$\rm ^{+0.09}_{-0.05}$ \\
CDFS-2528 & 9.76$\rm ^{+0.09}_{-0.07}$ &9.71$\rm ^{+0.16}_{-0.00}$ &--21.57 & --0.33 & 101 & 0.20$\rm ^{+0.05}_{-0.05}$ &0.06$\rm ^{+0.03}_{-0.01}$ \\
SSA22a-M38 & 11.01$\rm ^{+0.18}_{-0.41}$ &10.71$\rm ^{+0.19}_{-0.40}$ &--22.99 & 0.22 & 115 & 0.20$\rm ^{+0.05}_{-0.20}$ &0.63$\rm ^{+0.95}_{-0.45}$ \\
SSA22a-aug16M16 & 10.29$\rm ^{+0.20}_{-0.21}$ &10.15$\rm ^{+0.11}_{-0.28}$ &--22.32 & --0.23 & 42 & 0.06$\rm ^{+0.04}_{-0.06}$ &0.39$\rm ^{+0.39}_{-0.23}$ \\
\hline
\end{tabular}
}
\par
\smallskip
The following quantities are reported in each column:
Col.~1, object name;
Col.~2, stellar mass inferred by using the galaxy templates of BC03;
Col.~3, stellar mass inferred by using the galaxy templates of M05;
Col.~4, absolute B~magnitude;
Col.~5, rest-frame $U-V$~color;
Col.~6, star formation rate (by using BC03);
Col.~7, dust reddening affecting the stellar light, by using the attenuation curve of \cite{calzetti00};
Col.~8, age of the stellar population.
\end{table}