\begin{table}%T2
\par
  \caption{\label{datos_fir}\FIR\ and \FUV\ data for the WR~galaxy sample analyzed in this work. } 
\small%\centering
\par
  \begin{tabular}{l cccc c  c cc}
  \hline\hline\noalign{\smallskip}
 Galaxy  &   $f_{\rm 12~\mu m}$ &  $f_{\rm 25~\mu m}$ &   $f_{\rm 60~\mu m}$   &  $f_{\rm 100~\mu m}$  &  $F_{\rm FIR}$ & Reg. & $m_{\rm FUV}$ &  
$f_{\rm FUV}$  \\
         &  [Jy]   & [Jy]      &  [Jy]    & [Jy]    &   \tablefootmark{a}  & \tablefootmark{b} &[mag] & \tablefootmark{c}  \\ 
  \hline
HCG 31         &  0.110~$\pm$~0.020 & 0.580~$\pm$~0.040 &  3.92~$\pm$~0.31  & 5.84~$\pm$~0.47 & 2.01~$\pm$~0.16  &AC&14.97~$\pm$~0.06 & 7.54~$\pm$~0.44\\
               &                  &                 &                 &               &                &B& 16.80~$\pm$~0.09 & 3.32~$\pm$~0.26\\
               &                  &                 &                 &               &                &E& 18.01~$\pm$~0.08 & 0.456~$\pm$~0.035\\
               &                  &                 &                 &               &                &F& 18.24~$\pm$~0.11 & 0.460~$\pm$~0.047\\ 
               &                  &                 &                 &               &                &G& 15.93~$\pm$~0.06 & 3.11~$\pm$~0.18\\
               &                  &                 &                 &               &                &H& 20.63~$\pm$~0.40 & 0.0041~$\pm$~0.0014\\ 			   			     
Mkn 1087       &  0.103~$\pm$~0.029 & 0.414~$\pm$~0.058 &  3.03~$\pm$~0.33  & 4.44~$\pm$~0.40 & 1.54~$\pm$~0.16  &\nodata& \nodata&\nodata \\
Haro 15        &  0.118~$\pm$~0.034 & 0.297~$\pm$~0.089 &  1.36~$\pm$~0.12  & 1.97~$\pm$~0.20 & 0.690~$\pm$~0.064&\nodata& 15.12~$\pm$~0.07& 9.41~$\pm$~0.57\\
Mkn 1199       &  0.282~$\pm$~0.031 &  1.28~$\pm$~0.09  &  6.82~$\pm$~0.34  & 8.85~$\pm$~0.53 & 3.33~$\pm$~0.18  &\nodata& \nodata&\nodata \\
Mkn 5          &  $<$0.0503       &  $<$0.0533      &  0.21~$\pm$~0.04  & $<$0.8473     & $<$1.75        &\nodata& 17.76~$\pm$~0.07 & 1.59~$\pm$~0.10\\
IRAS 08208+2816&  0.126~$\pm$~0.029 & 0.278~$\pm$~0.067 &  1.15~$\pm$~0.09  & 1.70~$\pm$~0.17 & 0.588~$\pm$~0.051&\nodata& 16.59~$\pm$~0.07 & 3.75~$\pm$~0.23\\
IRAS 08339+6517&  0.250~$\pm$~0.025 &  1.13~$\pm$~0.02  & 5.81~$\pm$~0.04   & 6.48~$\pm$~0.09 & 2.71~$\pm$~0.02  & & 15.37~$\pm$~0.06 & 10.7~$\pm$~0.6\\
               &                  &                 &                 &               &                &c& 19.70~$\pm$~0.10 & 0.160~$\pm$~0.014\\
POX 4          &  $<$0.987        & 0.153~$\pm$~0.040 & 0.629~$\pm$~0.057 & $<$0.5798     & $<$0.278       &POX~4& 16.03~$\pm$~0.06 & 2.82~$\pm$~0.16\\
               &                  &                 &                 &               &                &Comp.& 19.06~$\pm$~0.12 & 0.269~$\pm$~0.030 \\
UM 420         &  \nodata         & $<$0.275           &    0.411:    &   0.613:      & 0.211:     &\nodata& 18.22~$\pm$~0.06 & 0.377~$\pm$~0.021\\
SBS 0926+606   &  $<$0.07553      &  $<$0.08818     & 0.269~$\pm$~0.046 & $<$0.5296     & $<$0.154       &A& 16.71~$\pm$~0.06 & 1.75~$\pm$~0.09\\
               &                  &                 &                 &               &                &B& 17.84~$\pm$~0.10 & 0.829~$\pm$~0.073\\ 	
SBS 0948+532   &  \nodata & \nodata& \nodata & \nodata                                & \nodata        &\nodata&  \nodata&\nodata \\
SBS 1054+365   &   $<$0.055     & $<$0.100  & 0.536~$\pm$~0.048 & 0.97~$\pm$~0.15         & 0.296~$\pm$~0.035&\nodata& 16.67~$\pm$~0.07 & 1.18~$\pm$~0.08 \\
SBS 1211+540   &  \nodata & \nodata& \nodata & \nodata                                & \nodata        &\nodata& 18.40~$\pm$~0.07 & 0.370~$\pm$~0.022\\
SBS 1319+579   &  \nodata & \nodata& 0.209: & 0.685:                                  & 0.154:         &\nodata& 17.00~$\pm$~0.06 & 0.864~$\pm$~0.048\\
               &                  &                 &                 &               &                & A     & 18.60~$\pm$~0.06 & 0.199~$\pm$~0.010\\           
SBS 1415+437   &  \nodata & \nodata& \nodata & \nodata                                & \nodata        &\nodata& 16.22~$\pm$~0.06 & 3.95~$\pm$~0.22\\
III Zw 107     &  $<$0.0968        & 0.336~$\pm$~0.050  & 1.37~$\pm$~0.20  & 1.72~$\pm$~0.31& 0.662~$\pm$~0.104&\nodata& \nodata&\nodata\\
Tol 9          &  0.111~$\pm$~0.030  & 0.465~$\pm$~0.051  & 2.71~$\pm$~0.22  & $<$5.516     & $<$1.58        &\nodata& 17.57~$\pm$~0.07& 4.22~$\pm$~0.22\\
Tol 1457-262   & $<$0.117          & 0.611~$\pm$~0.067  & 3.09~$\pm$~0.19  & 3.68~$\pm$~0.40& 1.47~$\pm$~0.11  &\nodata& 15.84~$\pm$~0.07& 6.95~$\pm$~0.47\\
               &                  &                 &                 &               &                &Obj~1& 16.15~$\pm$~0.06  & 5.26~$\pm$~0.29\\
               &                  &                 &                 &               &                &Obj~2& 17.41~$\pm$~0.13  & 1.64~$\pm$~0.18\\
               &                  &                 &                 &               &                &\#15& 19.71~$\pm$~0.21   & 0.199~$\pm$~0.037\\ 
Arp 252        &  0.188~$\pm$~0.023  & 0.994~$\pm$~0.050  & 3.91~$\pm$~0.20  & 4.11~$\pm$~0.25& 1.79~$\pm$~0.10  &A& 18.67~$\pm$~0.08 & 1.91~$\pm$~0.13\\
               &                   &                  &                &              &                &B& 18.84~$\pm$~0.07 & 0.441~$\pm$~0.027\\
NGC 5253       &  2.50~$\pm$~0.02    & 12.07~$\pm$~0.05   & 29.84~$\pm$~0.07 &30.08~$\pm$~0.21& 13.49~$\pm$~0.05 &\nodata& 12.81~$\pm$~0.06 & 123.0~$\pm$~6.5\\
	  \hline
  \end{tabular}
 \tablefoot{\tablefoottext{a}{In units of $10^{-10}$ erg s$^{-1}$ cm$^{-2}$.}\\
	  \tablefoottext{b}{Region within each system (HCG~31, IRAS~08339+6517, POX~4, SBS~0926+606, SBS~1319+579, Tol~1457-262, and Arp~252; see Paper~I). }\\ 
\tablefoottext{c}{In units of $10^{-14}$ erg s$^{-1}$ cm$^{-2}$ \AA$^{-1}$.  }
}
  \vspace*{4mm}
\end{table}