\begin{table}%t1
\caption{\label{galaxias}VIMOS LIRG sample: for each pointing, the total number of data points, mean value and standard deviation for the different line ratios and  velocity dispersion are given.} 
%%\centering

\par
\begin{tabular}{cccccccccccccccccccccccccc}
\hline \hline \noalign{\smallskip}
Galaxy &
$\log L_{\rm ir}^{(1)}$ &
$D$      &
Scale  &
\multicolumn{2}{c}{[N~\textsc{ii}]$\lambda$6584/H$\alpha$} &
\multicolumn{2}{c}{[S~\textsc{ii}]$\lambda\lambda$6717,6731/H$\alpha$} & 
\multicolumn{2}{c}{[O~\textsc{i}]$\lambda$6300/H$\alpha$}  &
\multicolumn{2}{c}{$\sigma^{(2)} $ (km s$^{-1}$)}\\
 (IRAS number) &
($L_\odot$) &
(Mpc) &
(pc/$^{\prime\prime}$) &
$n$ & $\overline x\pm\sigma (x)$ &
$n$ & $\overline x\pm\sigma (x)$ &
$n$ & $\overline x\pm\sigma (x)$ &
$n$ & $\overline x\pm\sigma (x)$ \\
\hline
\multicolumn{12}{c}{Class 0}\\
F06295$-$1735       & 11.27 & 92.7  & 431 & 
  998 & 0.38 $\pm$ 0.07 & 486 & 0.31 $\pm$ 0.06 & 194 & 0.05 $\pm$ 0.04 & 1118 & 33 $\pm$ 11\\
F06592$-$6313       & 11.91 & 100.0 & 464 &
  199 & 0.82 $\pm$ 0.32 &\ldots&\ldots&\ldots&\ldots& 266 & 54 $\pm$ 33\\
F07027$-$6011  N    & 11.64 & 137.4 & 626 &
  342 & 0.40 $\pm$ 0.09 &  94 & 0.30 $\pm$ 0.06 & 92 & 0.07 $\pm$ 0.04 & 387 & 32 $\pm$ 11\\
F07027$-$6011  S    &  & 137.4 & 626 &
  163 & 0.61 $\pm$ 0.17 &  74 & 0.24 $\pm$ 0.05 & 49 & 0.03 $\pm$ 0.02 & 177 & 72 $\pm$ 17\\
F07160$-$6215       & 11.16 & 46.7  & 221 &
  755 & 0.92 $\pm$ 0.61 & 189 & 0.33 $\pm$ 0.16  & \ldots&\ldots&  888 & 69 $\pm$ 37\\
F10015$-$0614       & 11.77 & 73.1  & 343 &
 1298 & 0.41 $\pm$ 0.10 & 850 & 0.31 $\pm$ 0.08  & 137 & 0.03 $\pm$ 0.01 & 1312 & 51 $\pm$ 13\\
F10409$-$4556       & 11.26 & 91.4  & 425 &
  928 & 0.49 $\pm$ 0.25 &\ldots&\ldots&\ldots&\ldots& 1083 & 39 $\pm$ 16\\
F10567$-$4310       & 11.07 & 74.6  & 350 &
 1154 & 0.44 $\pm$ 0.15 & 270 & 0.25 $\pm$ 0.06 & \ldots&\ldots& 1153 & 29 $\pm$ 11\\
F11255$-$4120       & 11.04& 70.9  & 333 &
  759 & 0.58 $\pm$ 0.28 & 173 & 0.28 $\pm$ 0.06 & \ldots&\ldots & 782 & 33 $\pm$ 20\\
F11506$-$3851       & 11.30& 46.6  & 221 &
  887 & 0.67 $\pm$ 0.23 & 434 & 0.33 $\pm$ 0.13 & 327 & 0.04 $\pm$ 0.03 & 914 & 41 $\pm$ 14\\
F12115$-$4656       & 11.11& 80.3  & 375 &
  724 & 0.52 $\pm$ 0.18 & 462 & 0.31 $\pm$ 0.08 & 274 & 0.03 $\pm$ 0.02 & 847 & 41 $\pm$ 12\\
F13229$-$2934       & 11.29 & 59.3  & 280 & 
  865 &  1.21 $\pm$ 0.71 & 295 & 0.42 $\pm$ 0.19 & 146 & 0.07 $\pm$ 0.06 & 932 &  65 $\pm$ 24\\
F22132$-$3705       & 11.22& 49.3  & 234 & 
 1706 & 0.41 $\pm$ 0.08 & 1490 & 0.29 $\pm$ 0.08 & 712 & 0.03 $\pm$ 0.02 &1714 & 32 $\pm$ 8\\
\hline
\multicolumn{12}{c}{Class 1}\\
F01159$-$4443       & 11.48 & 99.8  & 462 &
 558  & 0.45 $\pm$ 0.12 & 170 & 0.29 $\pm$ 0.06 & 97 & 0.07 $\pm$ 0.05 & 646 & 48 $\pm$ 20\\
ESO 297-G011       & 11.18 & 75.0  & 352 &
 1339 & 0.45 $\pm$ 0.11 & 627 & 0.32 $\pm$ 0.08 & 109& 0.03 $\pm$ 0.03 &1404 & 32 $\pm$ 10\\
ESO 297-G012       &  & 75.0  & 352 &
  223 & 0.54 $\pm$ 0.15 &  97 & 0.38 $\pm$ 0.10 &  80& 0.10 $\pm$ 0.08 & 226 & 91 $\pm$ 31\\
F06076$-$2139       & 11.67 & 165.0 & 743 &
  274 & 0.63 $\pm$ 0.45 &\ldots&\ldots&\ldots&\ldots&313 & 40 $\pm$ 25\\
F06259$-$4708 P1   & 11.91 & 171.1 & 769 & 
    443 & 0.48 $\pm$ 0.24 & 221 & 0.27 $\pm$ 0.10 & 149 & 0.04 $\pm$ 0.04 & 550 & 81 $\pm$ 40\\
F06259$-$4708 P2   &   & 171.1 & 769 &
    279 & 0.30 $\pm$ 0.08 & 201 & 0.36 $\pm$ 0.11 & 163 & 0.06 $\pm$ 0.05 & 404 & 59 $\pm$ 20\\
08424$-$3130        & 11.04 & 70.1  & 329 &
  241 & 0.80 $\pm$ 0.47 & 108 & 0.38 $\pm$ 0.15 &  56 & 0.05 $\pm$ 0.03 & 392 & 73 $\pm$ 32\\
F08520$-$6850       & 11.83 & 205.4 & 909 &
  196 & 0.34 $\pm$ 0.10 & 103 & 0.39 $\pm$ 0.10 &  39 & 0.05 $\pm$ 0.03 & 318 & 72 $\pm$ 31\\
IC 563$^{(3,4)}$        & 11.21 & 89.0  & 415 &
  873 & 0.36 $\pm$ 0.08 & 491 & 0.33 $\pm$ 0.10 & 264 & 0.04 $\pm$ 0.02 & 1007 & 38 $\pm$ 9\\
IC 564 P1$^{(3,4)}$     &  & 89.0  & 415 &
  727 & 0.42 $\pm$ 0.12 & 163 & 0.35 $\pm$ 0.12 &\ldots&\ldots & 843 & 33 $\pm$ 10\\
IC 564 P2 $^{(3,4)}$    &  & 89.0  & 415 &
  495 & 0.37 $\pm$ 0.08 & 77 & 0.27 $\pm$ 0.09  &\ldots&\ldots & 635 & 36 $\pm$ 14\\
12042$-$3140        & 11.37 & 101.1 & 468 &
  540 & 0.58 $\pm$ 0.23 & 246 & 0.33 $\pm$ 0.13 & 176 & 0.08 $\pm$ 0.06 & 611 &  85 $\pm$ 46\\
12596$-$1529        &  11.07 & 69.0  & 324 &
  433 & 0.42 $\pm$ 0.13 & 226 & 0.41 $\pm$ 0.14 & 35 & 0.03 $\pm$ 0.02 & 487 &  64 $\pm$ 34\\
F14544$-$4255 E     & 11.11 & 68.2  & 320 &
  322 & 0.45 $\pm$ 0.19 &  53 & 0.21 $\pm$ 0.06 & \ldots&\ldots& 370 & 55 $\pm$ 15\\ 
F14544$-$4255 W     &  & 68.2  & 320 & 
  356 & 0.70 $\pm$ 0.26 & 165 & 0.68 $\pm$ 0.27 & 87 & 0.15 $\pm$ 0.09 & 392 & 66 $\pm$ 24\\
18093$-$5744 N      & 11.57 & 75.3  & 353 & 
 804 & 0.41 $\pm$ 0.12 &  528 &0.36 $\pm$ 0.09&  105 &0.03 $\pm$ 0.02 & 886 &  46 $\pm$ 13\\
18093$-$5744 C      &  & 75.3  & 353 & 
 373 &0.23 $\pm$ 0.07&  204 &0.23 $\pm$ 0.11&  61 & 0.02 $\pm$ 0.01 & 634 &  80 $\pm$ 35\\
18093$-$5744 S      &  & 75.3  & 353 & 
 316 & 0.46 $\pm$ 0.10&  185 & 0.33 $\pm$ 0.06&   28 & 0.03 $\pm$ 0.02& 359 &  47 $\pm$ 16\\
\hline
\multicolumn{12}{c}{Class 2}\\
F04315$-$0840       &  11.69 & 69.1  & 325 &
  763 & 0.58 $\pm$ 0.24 & 398 & 0.42 $\pm$ 0.13 & 407 & 0.10 $\pm$ 0.08 & 759 & 66 $\pm$ 32\\
08355$-$4944        &  11.60 & 113.1 & 521 &
  260 & 0.32 $\pm$ 0.07 & 121 & 0.25 $\pm$ 0.06 & 108 & 0.03 $\pm$ 0.02 & 347 & 59 $\pm$ 20\\
F10038$-$3338       &  11.77 & 149.9 & 679 &
  172 & 0.60 $\pm$ 0.29 & 58 & 0.44 $\pm$ 0.18 & 42 & 0.13 $\pm$ 0.09 & 303 & 55 $\pm$ 28\\
10257$-$4338        &  11.69 & 40.4  & 192 &
 1698 & 0.45 $\pm$ 0.11 &1573 & 0.39 $\pm$ 0.13 & 1403 & 0.06 $\pm$ 0.05 &1744 & 61 $\pm$ 19\\
12116$-$5615$^{(3)}$ &  11.61 & 80.3  & 375 &
   90 & 0.84 $\pm$ 0.29 & 33  & 0.34 $\pm$ 0.13 & \ldots&\ldots & 114 & 70 $\pm$ 15\\
13001$-$2339$^{(3)}$ & 11.48 & 94.5  & 439 &
  320 & 0.78 $\pm$ 0.28 & 80  & 0.63 $\pm$ 0.16 &  96 & 0.21 $\pm$ 0.07 & 388 & 117 $\pm$ 54\\
17138$-$1017$^{(3)}$ & 11.41 & 75.2  & 352 &
  235 & 0.53 $\pm$ 0.15 &  87 & 0.38 $\pm$ 0.10 & \ldots&\ldots& 257 & 63 $\pm$ 18\\
21453$-$3511        & 11.41 & 70.0  & 329 &
 1112 & 0.61 $\pm$ 0.41 & 476 & 0.23 $\pm$ 0.11 &  63 & 0.04 $\pm$ 0.05 & 1136 & 43 $\pm$ 19\\
\hline
\end{tabular}
\tablefoot {\tablefoottext{1}{Logarithm of the infrared luminosity, $L_{\rm ir} = L(8{-}1000~\mu$m), in units of solar bolometric luminosity, calculated using the fluxed in the four IRAS bands as given in \citet{san03}, when available. Otherwise from the IRAS fluxes given in IRAS Point Source and Faint Source catalogs \citet{mos90}. When a system of more than one galaxy is observed using several VIMOS pointings, the infrared luminosity of the entire system is indicated in the data corresponding to the first galaxy of the system.}\\  
\tablefoottext{2}{Velocity dispersion derived from the H$\alpha$~line.}\\
\tablefoottext{3}{Classification uncertain. Not used in the analysis of systems grouped by interaction class.}\\
\tablefoottext{4}{Members of \object{IRAS~09437+0317}.}}
\vspace*{5.5mm}
\end{table}