\begin{table}%t5
\caption{\label{lum}Luminosities and star formation rates.}
%\centerline
 {\begin{tabular}{lccccccccl}
\hline\hline
Source & $z_{\rm phot}$ & $L_{\rm{1.4~GHz}}$$^{b}$           & $L_{\rm{FIR,mm}}$         & $L_{\rm{FIR,radio}}$$^{c}$ &      $SFR_{\rm{mm}}$$^{d}$&      $SFR_{\rm{radio}}$$^{d}$ & $\nu$$L_{\nu}$(1.6~$\mu$m)    & $M_{\star}$                                  & SMG/SFRG \\
       &            & (10$^{24}$~W~Hz$^{-1}$) &  \multicolumn{2}{c}{(10$^{12}$~$L_{\odot}$)} &  \multicolumn{2}{c}{($M_{\odot}$~yr$^{-1}$)} & (10$^{11}$~$L_{\odot}$) & \multicolumn{1}{c}{(10$^{11}$~$M_{\odot}$)} & \\
\hline
\vspace{0.4 ex}																	
L-1  &       1.92 &            1.60 & 4.63~$\pm$~1.04 &    3.27~$\pm$~0.81 &                      834 & 588 & 1.67 &   1.03 & SMG        \\	
\vspace{0.4 ex}																	
L-2  &       1.92 &            0.96 & \textless4.77 &    1.96~$\pm$~0.39 &             \textless859 & 353 & 1.61 &   1.08 & weak Radio? \\	
\vspace{0.4 ex}														 			
L-3  &       1.73 &            0.33 & \textless5.22 &  0.66~$\pm$~0.52 &  \textless941 & \textless284 & 1.66 & 1.13 & weak Radio \\	
\vspace{0.4 ex}																	
L-4  &       2.13 &            1.02 & \textless5.37 &    2.08~$\pm$~3.08 &    \textless966 & \textless1664 & 3.02 &   2.85 & SFRG?      \\	
\vspace{0.4 ex}																	
L-5  &       2.04 &            2.40 & 4.32~$\pm$~1.19 &    4.90~$\pm$~0.92 &                      777 & 883 & 2.53 &   1.36 & SMG?        \\	
\vspace{0.4 ex}																	
L-6  &       2.26 &            1.10 & \textless3.49 &  2.25~$\pm$~0.79 &           \textless627 & 405 & 2.07 & 1.07 & SFRG? \\	
\vspace{0.4 ex}																	
L-7  &       1.89 &            2.15 & \textless4.66 &  4.35~$\pm$~1.06 &                    \textless839 & 788 & 2.19 & 1.55 & ?      \\	
\vspace{0.4 ex}																	
L-8  &       2.42 &            3.80 & \textless4.24 &    [7.75~$\pm$~1.09] &             \textless763 & [1396] & 2.89 &   [1.52] & SFRG       \\	
\vspace{0.4 ex}																	
L-9  &       2.33 &            2.99 & 6.28~$\pm$~0.86 &    6.11~$\pm$~1.94 &                     1130 & 1100 & 2.71 &   2.66 & SMG        \\	
\vspace{0.4 ex}																	
L-10 &       2.45 &            1.56 & \textless4.73 &    3.19~$\pm$~1.05 &                      \textless851 & 574 & 4.01 &  2.31 & ?      \\	
\vspace{0.4 ex}																	
L-11 &       1.92 &            4.52 & 4.84~$\pm$~0.91 &  [9.21~$\pm$~3.63] &                   870 & [1658] & 1.57 & [0.78] & SMG        \\	
\vspace{0.4 ex}																	
L-12 &       1.71 &            1.56 & \textless5.71 &    3.19~$\pm$~1.12 &                    \textless1029 & 575 & 3.19 &   3.09 & ?       \\ 	
\vspace{0.4 ex}																	
L-13 &       2.22 &            0.86 & \textless4.95 &    1.75~$\pm$~0.89 &    \textless891 & 315 & 1.60 &   0.87 & weak Radio \\	
\vspace{0.4 ex}																	
L-14 &       2.36 &            5.53 & 3.34~$\pm$~1.11 &  [11.30~$\pm$~2.99] &                   602 & [2029] & 3.37 & [1.74] & SMG?        \\	
\vspace{0.4 ex}								 							
L-15 &       1.86 &            1.92 & 3.71~$\pm$~0.97 &    3.93~$\pm$~0.76 &                      667 & 707 & 3.09 &   3.21 & SMG?        \\	
\vspace{0.4 ex}								 									
L-16 &       1.73 &            1.36 & \textless4.05 & 2.77~$\pm$~1.51  & \textless729 & 499 & 1.34 &   0.92 & SFRG?       \\	
\vspace{0.4 ex}																	
L-17 &       1.90 &            7.90 & 3.52~$\pm$~1.00 & [16.12~$\pm$~2.70] &                   633 & [2902] & 2.27 & [1.07] & SMG?        \\	
\vspace{0.4 ex}																
L-18 &       1.85 &            1.60 & \textless3.82 &  3.27~$\pm$~0.86 &           \textless688 & 589 & 3.05 & 2.17 & SFRG       \\	
\vspace{0.4 ex}																	
L-19 &       1.69 &            1.08 & \textless4.57 &  2.21~$\pm$~0.53 &           \textless822 & 398 & 1.67 & 0.99 & ?      \\	
\vspace{0.4 ex}																	
L-20 &       2.69 &            4.98 & 4.18~$\pm$~1.22 &   10.20~$\pm$~0.95 &                      752 & 1830 & 5.68 &   7.16 & SMG?        \\	
\vspace{0.4 ex}																	
L-21 &       1.78 &            1.61 & 4.85~$\pm$~1.27 &    3.23~$\pm$~1.94 &                     873 & 592 & 1.74 &   1.12 & SMG?        \\	
\vspace{0.4 ex}																	
L-22 &       2.57 &            5.70 & 5.35~$\pm$~1.15 &   11.62~$\pm$~4.323 &                     964 & 2092 & 4.11 &   3.06 & SMG        \\	
\vspace{0.4 ex}																	
L-23 &       2.38 &            3.08 & 4.91~$\pm$~1.35 &    6.28~$\pm$~1.63 &                      885 & 1130 & 2.27 &   1.27 & SMG?        \\	
\vspace{0.4 ex}																
L-24 &       2.07 &            0.57 & \textless4.14 &    1.16~$\pm$~0.29 &    \textless746 & \textless209 & 1.82 &   1.02 & weak Radio \\	
\vspace{0.4 ex}																	
L-25 & 1.47$^{a}$ &            1.01 & 4.02~$\pm$~1.16 &    2.07~$\pm$~0.59 &                      723 & 372 & 1.29 &   0.84 & SMG?        \\	
\vspace{0.4 ex}														 			
L-26 &       1.72 &            0.73 & \textless4.05 &    1.49~$\pm$~1.07 & \textless729 & \textless579    & 1.55 & 1.57 & weak Radio      \\	
\vspace{0.4 ex}																	
L-27 &       2.20 &            1.41 & 3.89~$\pm$~1.15 &    2.87~$\pm$~0.96 &                      701 & 517 & 2.18 &   1.21 & SMG?        \\	
\vspace{0.4 ex}																	
L-28 &       1.88 &            0.48 & \textless4.65 &    0.98~$\pm$~0.20 &             \textless836 & \textless176 & 1.79 &   1.29 & ?       \\	
\vspace{0.4 ex}																	
L-29 &       1.93 &            0.77 & \textless4.62 &    1.58~$\pm$~0.68 &   \textless831 & 284 & 2.33 &   1.62 & weak Radio      \\	
\vspace{0.4 ex}																	
L-30 &       2.38 &            1.45 & \textless2.97 &    2.96~$\pm$~2.39 &    \textless534 & \textless1290 & 3.17 &   2.01 & SFRG      \\	
\vspace{0.4 ex}																	
L-31 &       2.74 &            3.13 & \textless4.43 &  6.39~$\pm$~3.43 &          \textless797 & 1150 & 3.65 & 1.37 & ?       \\	
\vspace{0.4 ex}																	
L-32 &       2.38 &            1.03 & \textless4.53~$\pm$~1.00 &   2.10~$\pm$~1.54 &            \textless815 & \textless278 & 2.77 &   1.84 & ?       \\	
\vspace{0.4 ex}																	
L-33 &       2.18 &            0.92 & \textless5.13 &  1.87~$\pm$~0.97 & \textless924 & 337 & 2.47 & 1.49 & weak Radio?      \\	
\hline
\end{tabular}}
\par
\smallskip
\par
$^a$ Spectroscopic redshift from \citet{Bert07a}.\\
$^b$ The value of $L_{\rm{1.4~GHz}}$, the rest-frame luminosity at 1.4~GHz, is the weighted average of the two determinations of $L_{\rm{1.4~GHz}}$ from 20~cm and 50~cm flux densities when both are available.\\
$^c$ The values of $L_{\rm{FIR,radio}}$, the infrared SFR derived from the radio flux densities and the stellar mass are dubious for sources with high 20~cm/1.2~mm flux densities ratios. They are reported, in brackets.\\
$^d$ SFR calculated by Kennicutt's formula (Eq.~(6)) with a Salpeter IMF (see text).\\
The upper limits of $L_{\rm{FIR,mm}}$ and SFR$_{\rm{mm}}$ are ``3$\sigma$'' limits, except for the sources with 1.5~$<$~{\it S/N}~$<$~3 where they are the observed value plus 2$\sigma$.\\ 
The upper limits of $L_{\rm{FIR,radio}}$ and {\it SFR}$_{\rm{radio}}$ are ``3$\sigma$'' limits. 
\end{table}