\begin{table}%t2 
\caption{Flux measurements for the FIRBACK South Marano sample. 
\label{results_M}} 
\par
%\centering
\par 
{
 \begin{tabular}{ccccccccccccccc} 
 \hline  \hline
   IR source&LIR &ID&$z$&$Av$&\multicolumn{2}{c}{$[{\rm OII}]_{ 
   3727}$}&H$\beta$&$[{\rm OIII}]_{4959}$ &$[{\rm OIII}]_{5007}$
   &\multicolumn{2}{c}{H$\alpha$}&$[{\rm NII}]_{6583}$&Nature&Comments\\
   (1)  &(2)    &(3)&(4)   &(5)&(6) &(7) &(6)  &(6)  &(6)  &(6)  &(7)  &(6)  &(8) &(9)\\
 \hline
FSM\_000& 10.9  &1* &0.0466&3.9&1.4 &256 &0.70 &--    &--    &13   &234  &3.6  &e+a&1 \& 2 interacting\\
	&       &2  &0.0462& -- & --  & --  & --   &--    & --   & --   & --   & --   &a   &\\
FSM\_001& 10.6	&1* &0.0297&4.6&0.89&410 & --   & --   &0.14 &5.6  &165  &1.1  &e+a&1 \& 2 interacting\\
	&	&2  &0.0289& -- &0.54&26  & --   & --   & --   & --   & --   &0.99 &a   &\\
FSM\_002& 10.4	& * &0.0310&4.3&0.88&269 & --   & --   & --   &4.2  &98   &0.43 &e+a&\\
FSM\_003& 11.8	& * &0.1309&7.1&0.21&2750& --   & --   &0.15 &1.96 &360  &1.1  &e+a&LINER ?\\
FSM\_004& 11.3	& * &0.0782&3.4&4.9 &476 &1.3  &9.2  &24   &11.8 &147  &5.6  &agn &\\
FSM\_005& 9.6	&1* &0.1505& -- &0.52&25  & --   &0.21 &0.30 &3.9  &32   &0.81 &e+a&FSM\_005 $=1+2$\\
	&	&2* &0.1516& -- &0.19&9.2 & --   &0.22 & --   &1.8  &15   & --   &e+a&1 \& 2 merging\\
FSM\_006&	&1  &0.0480&2.6&0.29&9.1 & --   &0.071&0.13 &0.28 &1.8  & --   &e+a&\\
	& 12.1	&2* &0.2050&2.0&0.68&10  &0.22 &0.087&0.13 &3.5  &15.4 &0.4  &e+a&\\
FSM\_007& 11.2	&*  &0.0923&2.6&1.5 &52  &0.71 &0.29 &0.48 &7.7  &53   &2.3  &e   &\\
FSM\_008& 12.2	&*  &0.2282&2.1&0.34&5.4 &0.18 &0.063&0.23 &2.2  &9.9  &0.92 &e+a&\\
FSM\_009& 11.9	&1* &0.1918&2.0&0.63&9.5 &--    &0.067&0.18 &1.9  &8.3  &0.45 &e+a&interacting with 2\\
	&	&2  &0.1915&2.1&0.23&3.9 & --   & --   & --   &0.56 &2.6  & --   &e+a&\\
FSM\_010& 12.2	&1* &0.2569& -- & --  & --  & --   & --   & --   & --   & --   & --   &a   &FSM\_010 $=1+2$\\
	&	&2* &0.2578&1.5&0.25&1.9 &0.082&0.019&0.051&0.72 &2.2  &0.30 &e+a&1 \& 2 interacting?\\
FSM\_011& 12.9	& * &0.6576& -- &0.95&45  &0.75 &1.5  &4.7  & --   & --   & --   &agn &pointlike\\
FSM\_012& 12.1  &1* &0.1925&2.5&1.2 &33  &0.43 &0.12 &0.36 &5.0  &31   &1.6  &e+a&\\
	&	&2  &0.0547&4.1&0.79&196 & --   & --   & --   &1.4  &29   &0.15 &e+a&\\
FSM\_013&	&1  &0.0546&1.8&0.40&4.6 & --   & --   &0.15 &0.51 &1.97 &0.030&e+a&\\
	& 12.2	&2* &0.2389&2.2&0.16&3.1 & --   & --   &0.09 &0.46 &2.3  &0.085&e+a&FSM\_013 $=2+3$\\
	&       &3* &0.2541&2.7&0.17&6.5 &0.077&0.14 &0.16 &0.43 &3.2  &0.61 &e+a&LINER ?\\
FSM\_014&11.5(A)&1* &0.1579& -- &0.49&23  &0.092&0.071&0.16 &0.27 &2.3  & --   &e+a&IR flux shared A $=1+2$\\
	&	&2* &0.1589& -- &0.61&29  &0.22 &0.10 &0.22 &0.43 &3.6  & --   &e+a&1 \& 2 interacting\\
	&11.8(B)&3* &0.2915&1.6&0.23&2.1 & --   & --   & --   &0.48 &1.6  &0.28 &e+a&IR flux shared B $=3$\\
FSM\_015&10.8	& * &0.0578&3.9&0.31&56  & --   & --   & --   &0.76 &13   &0.12 &e+a&\\
FSM\_016&11.5	& * &0.1302&3.3&0.50&43  &0.53 &0.079&0.15 &8.3  &96   &0.79 &e+a&\\
FSM\_017&11.0	&1* &0.0744&5.4&0.47&685 & --   & --   &0.091&1.9  &104  & --   &e+a&\\
	&	&2  &0.1295&2.7&0.22&8.2 &0.053& --   &0.081&0.31 &2.3  & --   &e+a&\\
	&	&3  &0.2991& -- &0.17&8.2 &0.089& --   & --   &0.17 &1.5  & --   &e+a&\\
FSM\_018&12.0	&1  &0.2329& -- & --  & --  & --   & --   & --   & --   & --   & --   &a   &\\
	&	&2  &0.2341& -- & --  & --  & --   & --   & --   & --   & --   & --   &a   &\\
FSM\_019&	&1  &0.0725&2.7&0.65&26  &0.084&0.14 &0.084&3.6  &27   & --   &e+a&\\ 
	&12.3	&2* &0.2568&2.2&0.13&2.7 & --   & --   & --   &0.75 &3.9  & --   &e+a&\\
FSM\_020&11.0	&1* &0.0714&2.5&1.2 &35  & --   &0.29 &0.27 &5.3  &33   &0.93 &e+a&1 \& 2 interacting\\
	&	& 2 &0.0713&1.3&1.5 &8.7 &0.32 &0.35 &1.0  &2.0  &5.2  & --   &e+a&\\
CFSM\_026&10.9	&*  &0.0780&4.7& --  & --  & --   & --   & --   &2.0  &66   & --   &e+a&\\
CFSM\_035&12.5	&*  &0.5902& -- &0.49&23  &4.1  & --   &1.6  & --   & --   & --   &agn &pointlike\\
CFSM\_039&10.9(A)&1*&0.1413&1.3&1.4 &8.0 &0.38 &0.36 &0.88 &2.8  &7.2  &0.67 &e+a&IR flux shared  A $=1$\\
	&11.7(B)&2* &0.2684&2.2&0.18&3.7 &0.098& --   & --   &1.2  &6.5  &0.44 &e+a&IR flux shared B $=2$\\ \hline
 \end{tabular}}
 { 
 \begin{tabular}{ll} 
(1) Name of FSM 170 $\mu$m published source.&(2) log10 of total IR luminosity 
   in $L_\odot$ (see Sect.~4.5).\\ 
(3) Identification number of the optical object. *: Object considered to be 
   the IR source.&(4) Redshift measured 
   from lines, error $\simeq$$5 \times 10^{-4}$ (see Sect.~2.4).\\ 
(5) Extinction $A_V = R\times E(B-V)$, from 
   Balmer decrement (Sect.~3.3), with $R = 3.2$. & 
(6) Main emission lines fluxes,
$10^{-15}~{\rm erg/s/cm^2}$, error $<$10\%. \\
(7) Flux corrected from absorption by star \& dust
extinction, $10^{-15}~{\rm erg/s/cm^2}$ (Sect.~3.3). & (8) Spectral
type. $e+a$: emission and absorption lines. $a$: no emission line.\\
\multicolumn{2}{l}{(9) Comments. IR flux can be attributed to two
optical objects, see source identification (Sect.~2.5).}\\
 \end{tabular}} 	
\end{table}