\begin{table}
%\centering
\par
\caption{\label{wrgfotb_ce} {Results for the broad-band optical/\NIR\ photometry of our WR galaxies sample. $E(B-V)$ was determined from the \CHb\ calculated from our optical spectra. All magnitudes and colors have been corrected for extinction; optical colors have been also corrected for the emission of the ionized gas. Except for NGC~5253, absolute magnitudes were computed using the distances provided by our optical spectra. See figures for the identification of the different regions inside galaxies.}}
{\tiny \begin{tabular}{l ccc rrr rrr}
\hline\hline
\noalign{\smallskip}
{\bf Object}     &   $E(B-V)$ &   $m_B$        &   $M_B$        &  $U-B$    &   $B-V$   &  $V-R$      & $V-J$     & $J-H$    & $H-K_{\rm s}$ \\ 
\hline
\noalign{\smallskip}
{\bf HCG 31}$^d$ \\
AC$^{c,d}$& 0.06~$\pm$~0.02 & 14.17~$\pm$~0.05  & $-$19.43~$\pm$~0.05 & $-$0.60~$\pm$~0.06 &    0.03~$\pm$~0.08 &    0.12~$\pm$~0.08 & 0.20~$\pm$~0.10 & 0.13~$\pm$~0.10 & 0.15~$\pm$~0.12\\ 	
B$^c$     & 0.18~$\pm$~0.04 & 14.89~$\pm$~0.05  & $-$18.71~$\pm$~0.05 & $-$0.38~$\pm$~0.08 &    0.17~$\pm$~0.06 &    0.06~$\pm$~0.06 & 0.14~$\pm$~0.10 & 0.13~$\pm$~0.10 & 0.12~$\pm$~0.10\\
E$^c$     & 0.06~$\pm$~0.03 & 17.84~$\pm$~0.06  & $-$15.76~$\pm$~0.06 & $-$0.65~$\pm$~0.10 & $-$0.03~$\pm$~0.10 &    0.20~$\pm$~0.09 & 0.29~$\pm$~0.12 & 0.05~$\pm$~0.10 & 0.18~$\pm$~0.12	\\
F1$^c$    & 0.20~$\pm$~0.03 & 17.84~$\pm$~0.06  & $-$15.76~$\pm$~0.06 & $-$0.99~$\pm$~0.12 & $-$0.07~$\pm$~0.12 & $-$0.04~$\pm$~0.10 &$-$0.17~$\pm$~0.14&0.04~$\pm$~0.17 & 0.29~$\pm$~0.30 \\
F2$^c$    & 0.09~$\pm$~0.03 & 19.26~$\pm$~0.06  & $-$14.34~$\pm$~0.06 & $-$1.01~$\pm$~0.12 & $-$0.09~$\pm$~0.12 & $-$0.02~$\pm$~0.10 & 0.01~$\pm$~0.16 & 0.08~$\pm$~0.30 & 0.20~$\pm$~0.50	\\
G$^c$     & 0.06~$\pm$~0.03 & 14.72~$\pm$~0.05  & $-$18.88~$\pm$~0.05 & $-$0.43~$\pm$~0.09 & $-$0.01~$\pm$~0.08 &    0.14~$\pm$~0.08 & 0.45~$\pm$~0.08 & 0.12~$\pm$~0.10 & 0.13~$\pm$~0.10 \\
AC$_{UC}$ & 0.06~$\pm$~0.02 & \nodata & \nodata                   & $-$0.38~$\pm$~0.12 &    0.19~$\pm$~0.10 &    0.29~$\pm$~0.12 & 0.69~$\pm$~0.14 & 0.53~$\pm$~0.16 & 0.17~$\pm$~0.16 \\
B$_{UC}$ & 0.18~$\pm$~0.04 & \nodata & \nodata                    & $-$0.27~$\pm$~0.12 &    0.31~$\pm$~0.08 &    0.23~$\pm$~0.08 & 0.72~$\pm$~0.10 & 0.61~$\pm$~0.14 & 0.19~$\pm$~0.16 \\
G$_{UC}$ & 0.06~$\pm$~0.02 & \nodata & \nodata                    & $-$0.33~$\pm$~0.10 &    0.28~$\pm$~0.08 &    0.30~$\pm$~0.08 & 0.79~$\pm$~0.10 & 0.52~$\pm$~0.14 & 0.23~$\pm$~0.16 \\
\hline
\noalign{\smallskip}
{\bf Mkn 1087}$^d$ & 0.17$^a$  & 13.08~$\pm$~0.04 & $-$22.15~$\pm$~0.04 &	$-$0.41~$\pm$~0.08 &0.17~$\pm$~0.08&0.20~$\pm$~0.08 &	0.52~$\pm$~0.06 &	0.20~$\pm$~0.06  
&	0.16~$\pm$~0.06 \\
C$^c$   & 0.14~$\pm$~0.02 &  14.62~$\pm$~0.03 & $-$20.61~$\pm$~0.03	& $-$0.57~$\pm$~0.06 & $-$0.02~$\pm$~0.06 &	0.11~$\pm$~0.06 &	0.31~$\pm$~0.10 &	 
0.15~$\pm$~0.10 &	0.15~$\pm$~0.10\\
N Comp$^c$  & 0.10~$\pm$~0.02 & 17.17~$\pm$~0.03 & $-$18.06~$\pm$~0.03 &	\nodata &  $-$0.05~$\pm$~0.06 &	 0.14~$\pm$~0.10 & 0.21~$\pm$~0.08 & 0.18~$\pm$~0.08 &  
0.13~$\pm$~0.08\\
\#1 &	0.07$^a$ &	18.89~$\pm$~0.05 & $-$16.34~$\pm$~0.05 & $-$0.75~$\pm$~0.15 & $-$0.01~$\pm$~0.10 &	0.10~$\pm$~0.08 & \nodata & \nodata & \nodata \\	
\#3	&   0.07$^a$ &  18.03~$\pm$~0.03 & $-$17.20~$\pm$~0.03 &    0.08~$\pm$~0.30 &    0.11~$\pm$~0.06	&   0.26~$\pm$~0.06 & 0.64~$\pm$~0.10 &	0.50~$\pm$~0.20 &  
\nodata \\	
UC & 0.17$^a$ & \nodata & \nodata        & \nodata &    0.27~$\pm$~0.08 &    0.29~$\pm$~0.08 & 0.82~$\pm$~0.10 & 0.59~$\pm$~0.14 & 0.27~$\pm$~0.16 \\
\hline
\noalign{\smallskip}
{\bf Haro 15}$^c$  & 0.11$^a$      & 13.82~$\pm$~0.04 & $-$20.87~$\pm$~0.04 & $-$0.52~$\pm$~0.08 & 0.26~$\pm$~0.08 &   0.32~$\pm$~0.08 & 0.17~$\pm$~0.08 & 0.58~$\pm$~0.08 & 0.22~$\pm$~0.08 \\
A$^c$      & 0.23~$\pm$~0.02 & 17.56~$\pm$~0.04 & $-$17.13~$\pm$~0.04 & $-$0.86~$\pm$~0.10 &$-$0.10~$\pm$~0.08& 0.13~$\pm$~0.08 & 0.20~$\pm$~0.08 & 0.24~$\pm$~0.08 & 0.18~$\pm$~0.10 \\
B       & 0.04~$\pm$~0.02 & 17.72~$\pm$~0.04 & $-$16.97~$\pm$~0.04 & $-$0.39~$\pm$~0.10 & 0.39~$\pm$~0.08 &   0.32~$\pm$~0.08 & 0.54~$\pm$~0.10 & 0.47~$\pm$~0.08 & 0.2~$\pm$~0.1       \\
C$^c$   & 0.08~$\pm$~0.02 & 14.76~$\pm$~0.04 & $-$19.93~$\pm$~0.04 & $-$0.52~$\pm$~0.08 & 0.29~$\pm$~0.08 &   0.31~$\pm$~0.08 & 0.25~$\pm$~0.08 & 0.38~$\pm$~0.08 & 0.22~$\pm$~0.08       \\
UC & 0.11$^a$ & \nodata & \nodata    & $-$0.29~$\pm$~0.10 &   0.44~$\pm$~0.08  &  0.37~$\pm$~0.08 & 0.98~$\pm$~0.10 & 0.56~$\pm$~0.14 & 0.22~$\pm$~0.18 \\
\hline
\noalign{\smallskip}
{\bf Mkn 1199}$^c$& 0.15$^a$      & 12.98~$\pm$~0.03 & $-$20.68~$\pm$~0.03 & $-$0.44~$\pm$~0.06 &    0.46~$\pm$~0.06 &    0.29~$\pm$~0.06 &   1.30~$\pm$~0.07 &  0.55~$\pm$~0.08 & 0.34~$\pm$~0.08 \\
MB            & 0.21~$\pm$~0.02 & 12.99~$\pm$~0.04 & $-$20.67~$\pm$~0.04 & $-$0.53~$\pm$~0.08 &    0.41~$\pm$~0.08 &    0.17~$\pm$~0.08 &   1.12~$\pm$~0.08 &  
0.55~$\pm$~0.08 & 0.33~$\pm$~0.08 \\ 
Center (C)    & 0.21~$\pm$~0.02 & 13.56~$\pm$~0.04 & $-$20.10~$\pm$~0.04 & $-$0.63~$\pm$~0.08 &    0.24~$\pm$~0.08 &    0.15~$\pm$~0.08&   1.17~$\pm$~0.08 &   0.44~$\pm$~0.08 & 0.26~$\pm$~0.08 \\
NE            & 0.11~$\pm$~0.02 & 16.09~$\pm$~0.04 & $-$17.57~$\pm$~0.04 &    0.16~$\pm$~0.08 &    0.51~$\pm$~0.08 &    0.34~$\pm$~0.08 &   1.29~$\pm$~0.08 &   
0.62~$\pm$~0.10 & 0.20~$\pm$~0.12 \\
NE c          & 0.11~$\pm$~0.02 & 18.12~$\pm$~0.04 & $-$15.54~$\pm$~0.04 & $-$0.45~$\pm$~0.08 &    0.28~$\pm$~0.08 &    0.25~$\pm$~0.08 &   \nodata       &   
\nodata       & \nodata \\
e               & 0.12~$\pm$~0.03$^d$& 18.99~$\pm$~0.05 & $-$14.67~$\pm$~0.05 & $-$0.50~$\pm$~0.10 &    0.39~$\pm$~0.10 &    0.15~$\pm$~0.10 &   \nodata       &   
\nodata       & \nodata \\
UC & 0.15$^a$ & \nodata & \nodata  & $-$0.12~$\pm$~0.12  &  0.51~$\pm$~0.08 &    0.31~$\pm$~0.08 & 1.22~$\pm$~0.12 &    0.65~$\pm$~0.16 &   0.32~$\pm$~0.18 \\
\hline
\noalign{\smallskip}
{\bf Mkn 5}   & 0.20~$\pm$~0.02$^a$ & 14.83~$\pm$~0.03 & $-$15.57~$\pm$~0.03 & $-$0.41~$\pm$~0.06 &    0.44~$\pm$~0.06 &	0.30~$\pm$~0.06  & 0.81$^e$&0.52~$\pm$~0.03$^e$&0.38~$\pm$~0.04$^e$\\
Main Body       & 0.20~$\pm$~0.02$^a$ & 15.46~$\pm$~0.04 & $-$14.94~$\pm$~0.04 & $-$0.57~$\pm$~0.08 &    0.39~$\pm$~0.08 &    0.21~$\pm$~0.08 & \nodata        &  
\nodata	& \nodata	 \\
A$^c$           & 0.18~$\pm$~0.02 & 16.54~$\pm$~0.04 & $-$13.86~$\pm$~0.04 & $-$0.81~$\pm$~0.08 &    0.10~$\pm$~0.08 &   0.12~$\pm$~0.08 & \nodata        &  
\nodata	& \nodata	 \\
B$^d$           & 0.21~$\pm$~0.02 & 19.13~$\pm$~0.04 & $-$11.27~$\pm$~0.04 & $-$0.48~$\pm$~0.08 &    0.29~$\pm$~0.08 &	0.09~$\pm$~0.08 & \nodata        &  
\nodata	& \nodata	 \\
c               & 0.20~$\pm$~0.02$^a$ & 20.14~$\pm$~0.04 & $-$10.26~$\pm$~0.04 & $-$0.17~$\pm$~0.08 &    0.43~$\pm$~0.08 &	0.27~$\pm$~0.08 & \nodata        &  
\nodata	& \nodata	 \\
UC          &     0.20~$\pm$~0.02$^a$  &  \nodata & \nodata & \nodata       & 0.45~$\pm$~0.08 &  0.30~$\pm$~0.08 & \nodata & \nodata &\nodata \\
\hline
\noalign{\smallskip}
{\bf IRAS 08208+2816}$^c$ & 
           0.17~$\pm$~0.02$^a$& 15.10~$\pm$~0.03& $-$21.29~$\pm$~0.03 & $-$0.49~$\pm$~0.06 &   0.22~$\pm$~0.06 &   0.35~$\pm$~0.08 &   1.03~$\pm$~0.08 &  
0.54~$\pm$~0.08 &    0.22~$\pm$~0.10 \\
\#1$^c$  & 0.30~$\pm$~0.03 & 19.15~$\pm$~0.04 & $-$17.24~$\pm$~0.04 & $-$0.52~$\pm$~0.08 &   0.19~$\pm$~0.06 &   0.30~$\pm$~0.12 &      \nodata   & \nodata      
&  \nodata         \\
\#2$^c$  & 0.30~$\pm$~0.03 & 19.22~$\pm$~0.05 & $-$17.17~$\pm$~0.05 & $-$0.55~$\pm$~0.08 &   0.19~$\pm$~0.06 &   0.19~$\pm$~0.12 &      \nodata   & \nodata       
&  \nodata         \\
\#3$^c$  & 0.33~$\pm$~0.02 & 16.80~$\pm$~0.03 & $-$19.59~$\pm$~0.03 & $-$0.50~$\pm$~0.08 &   0.05~$\pm$~0.06 &   0.05~$\pm$~0.12 &   0.80~$\pm$~0.12 & 
0.51~$\pm$~0.14 &    0.26~$\pm$~0.16 \\
\#5$^c$  & 0.28~$\pm$~0.02 & 17.83~$\pm$~0.03 & $-$18.56~$\pm$~0.03 & $-$0.65~$\pm$~0.08 &   0.07~$\pm$~0.06 &   0.08~$\pm$~0.12 &      \nodata   & \nodata      
&  \nodata         \\
\#6(C)$^c$  & 0.08~$\pm$~0.02 & 16.91~$\pm$~0.03 & $-$19.48~$\pm$~0.03 & $-$0.61~$\pm$~0.06 &    0.02~$\pm$~0.06 &   0.24~$\pm$~0.08 &   0.57~$\pm$~0.10 & 
0.27~$\pm$~0.08 &    0.18~$\pm$~0.10 \\
\#7$^c$  & 0.10~$\pm$~0.02 & 20.60~$\pm$~0.03 & $-$15.79~$\pm$~0.03 & $-$0.44~$\pm$~0.06 &    0.37~$\pm$~0.06 &	0.39~$\pm$~0.08 &      \nodata   & \nodata     
&  \nodata         \\
\#8$^c$  & 0.12~$\pm$~0.02 & 17.84~$\pm$~0.03 & $-$18.55~$\pm$~0.03 & $-$0.31~$\pm$~0.06 &    0.30~$\pm$~0.06 &	0.31~$\pm$~0.08 &  1.05~$\pm$~0.12  & 
0.53~$\pm$~0.12 &    0.28~$\pm$~0.14 \\
\#9$^c$  & 0.10~$\pm$~0.02 & 18.42~$\pm$~0.05 & $-$17.97~$\pm$~0.05 & $-$0.20~$\pm$~0.06 &    0.32~$\pm$~0.06 &	0.32~$\pm$~0.08 &      \nodata   & \nodata	& 
\nodata	   \\
\#10$^c$  & 0.08~$\pm$~0.02 & 18.04~$\pm$~0.04 & $-$18.35~$\pm$~0.04 & $-$0.20~$\pm$~0.06 &    0.29~$\pm$~0.06 &	0.35~$\pm$~0.08 &      \nodata   & \nodata	&
\nodata	   \\
\hline
\noalign{\smallskip}
{\bf IRAS 08339+6517}$^{c,d}$ & 
          0.16~$\pm$~0.02 & 12.94~$\pm$~0.04 & $-$21.57~$\pm$~0.04 & $-$0.51~$\pm$~0.08 & 0.01~$\pm$~0.08 & 0.26~$\pm$~0.08 & 1.36~$\pm$~0.06$^e$ & 
0.64~$\pm$~0.05$^e$ &	0.23~$\pm$~0.06$^e$\\
Companion$^d$  & 0.13~$\pm$~0.02 & 16.31~$\pm$~0.04	& $-$18.21~$\pm$~0.04 & $-$0.16~$\pm$~0.10 & 0.20~$\pm$~0.08 & 0.26~$\pm$~0.08 & 1.45~$\pm$~0.12$^e$ & 
0.21~$\pm$~0.25$^e$ &	0.68~$\pm$~0.28$^e$ \\
\hline
%\noalign{\smallskip}
{\bf POX 4}$^c$     & 0.06$^d$      & 14.56~$\pm$~0.01 & $-$18.79~$\pm$~0.01 & $-$0.68~$\pm$~0.03 &    0.29~$\pm$~0.02 &	0.32~$\pm$~0.04 &    0.42~$\pm$~0.08 
&   0.28~$\pm$~0.08 &  0.15~$\pm$~0.10  \\
\#3$^c$             & 0.06$^d$      & 17.88~$\pm$~0.01 & $-$15.41~$\pm$~0.01 & $-$1.00~$\pm$~0.03 & $-$0.06~$\pm$~0.02 &	0.04~$\pm$~0.04 &    0.12~$\pm$~0.10 
&   \nodata	   &	\nodata      \\
\#6$^c$             & 0.06$^d$      & 18.49~$\pm$~0.02 & $-$14.80~$\pm$~0.02 & $-$0.98~$\pm$~0.04 & $-$0.01~$\pm$~0.04 &	0.06~$\pm$~0.06 &    0.08~$\pm$~0.12 
&   \nodata	   &	\nodata      \\
\#7$^c$             & 0.06$^d$      & 20.69~$\pm$~0.02 & $-$12.60~$\pm$~0.02 & $-$0.88~$\pm$~0.04 & $-$0.09~$\pm$~0.06 &	0.11~$\pm$~0.08 &    \nodata	 &  
\nodata	   &	\nodata      \\
\#9 (C)$^c$    & 0.06~$\pm$~0.02              & 15.32~$\pm$~0.01 & $-$17.97~$\pm$~0.01 & $-$0.93~$\pm$~0.03 &    0.32~$\pm$~0.02 &    0.10~$\pm$~0.04 &	  
0.16~$\pm$~0.12 &   0.2:	   &    0.2:	     \\
\#11$^c$            & 0.06$^d$      & 19.19~$\pm$~0.04 & $-$14.10~$\pm$~0.04 & $-$0.65~$\pm$~0.06 &    0.07~$\pm$~0.02 &    0.15~$\pm$~0.04 &	   0.49~$\pm$~0.14 
&   \nodata	   &    \nodata	     \\
Comp       & 0.12       & 17.93~$\pm$~0.03 & $-$15.36~$\pm$~0.03 & $-$0.02~$\pm$~0.06 &    0.25~$\pm$~0.02 &    0.30~$\pm$~0.04 &	   0.87~$\pm$~0.10 &   0.7: &    0.3:	     \\
\hline
\noalign{\smallskip}
{\bf UM 420}  & 0.06~$\pm$~0.01 & 17.32~$\pm$~0.03 & $-$19.55~$\pm$~0.03 & $-$0.80~$\pm$~0.06 &    0.31~$\pm$~0.06 & 0.13~$\pm$~0.06$^d$&  0.77~$\pm$~0.12 &  
0.41~$\pm$~0.12 &    0.12~$\pm$~0.16 \\
      C$^c$& 0.06~$\pm$~0.01 & 19.35~$\pm$~0.03 & $-$17.52~$\pm$~0.03 & $-$1.00~$\pm$~0.06 &    0.11~$\pm$~0.06 &    0.18~$\pm$~0.06 &  0.38~$\pm$~0.12 &  
0.32~$\pm$~0.12 &    0.13~$\pm$~0.16 \\
      UGC 1809  & 0.04$^b$      & 15.02~$\pm$~0.03 & $-$19.92~$\pm$~0.03$^e$& 0.12~$\pm$~0.06 &    0.49~$\pm$~0.06 &    0.50~$\pm$~0.06 &  1.40~$\pm$~0.10 & 
0.68~$\pm$~0.12 &    0.28~$\pm$~0.14 \\      
\hline
\noalign{\smallskip}
{\bf SBS 0926+606 A}$^c$  & 0.08~$\pm$~0.02 & 16.45~$\pm$~0.03 & $-$17.29~$\pm$~0.03 & $-$0.75~$\pm$~0.06 &    0.01~$\pm$~0.06 &	0.14~$\pm$~0.06 & 0.54~$\pm$~0.06 &  0.21~$\pm$~0.06 &    0.15~$\pm$~0.08 \\
        A1$^c$  & 0.08~$\pm$~0.02 & 17.51~$\pm$~0.03 & $-$16.23~$\pm$~0.03 & $-$0.77~$\pm$~0.06 & $-$0.02~$\pm$~0.06 &	0.10~$\pm$~0.06 &  0.34~$\pm$~0.08 & 
0.18~$\pm$~0.08 &    0.11~$\pm$~0.08 \\
        A2$^c$  & 0.08~$\pm$~0.02 & 17.92~$\pm$~0.03 & $-$15.82~$\pm$~0.03 & $-$0.84~$\pm$~0.06 & $-$0.05~$\pm$~0.06 &	0.08~$\pm$~0.06 &  0.29~$\pm$~0.08 &  
0.18~$\pm$~0.08 &    0.12~$\pm$~0.08 \\
   A$_{UC}$     & 0.08~$\pm$~0.02 & 19.15~$\pm$~0.04 & $-$14.59~$\pm$~0.04 & $-$0.20~$\pm$~0.10 &    0.25~$\pm$~0.08 &	0.32~$\pm$~0.08 &  0.98~$\pm$~0.10 & 
0.57~$\pm$~0.10 &    0.16~$\pm$~0.12 \\
\noalign{\smallskip}
{\bf SBS 0926+606 B}$^c$  & 0.12~$\pm$~0.02 & 16.37~$\pm$~0.04 & $-$17.37~$\pm$~0.04 & $-$0.51~$\pm$~0.08 &    0.08~$\pm$~0.06 &	0.20~$\pm$~0.06 & 
0.83~$\pm$~0.06 &  0.29~$\pm$~0.06 &    0.18~$\pm$~0.08 \\
\hline
        Bc$^c$  & 0.12~$\pm$~0.02 & 18.84~$\pm$~0.04 & $-$14.90~$\pm$~0.04 & $-$0.87~$\pm$~0.08 &    0.04~$\pm$~0.06 &	0.11~$\pm$~0.06 &  0.52~$\pm$~0.12 & 
\nodata       &   \nodata        \\
 B$_{MB}^c$   & 0.12~$\pm$~0.02 & 17.21~$\pm$~0.03 & $-$16.53~$\pm$~0.03 & $-$0.54~$\pm$~0.06 &    0.13~$\pm$~0.06 &	0.16~$\pm$~0.06 &  0.75~$\pm$~0.06 & 
0.20~$\pm$~0.06 &    0.16~$\pm$~0.08 \\
 B$_{d}^c$  & 0.12~$\pm$~0.02 & 21.60~$\pm$~0.12 & $-$12.14~$\pm$~0.12 & $-$0.58~$\pm$~0.20 &    0.06~$\pm$~0.12 &	0.10~$\pm$~0.08 &  0.80~$\pm$~0.20 & \nodata      
&   \nodata        \\  
 B$_{UC}$       & 0.12~$\pm$~0.02 & 16.69~$\pm$~0.04 & $-$17.05~$\pm$~0.04 & $-$0.33~$\pm$~0.10 &    0.30~$\pm$~0.08 &	0.29~$\pm$~0.08 &  1.10~$\pm$~0.10 &
0.53~$\pm$~0.10 &    0.13~$\pm$~0.12 \\
\noalign{\smallskip}
  X  & 0.03$^b$    &  24.4:$^d$     &\nodata &\nodata      &  2.4:      & 1.4~$\pm$~0.2    & 4.4~$\pm$~0.2     & 1.07~$\pm$~0.14  &  0.65~$\pm$~0.18   \\  
\hline
\noalign{\smallskip}
{\bf  SBS 0948+532}$^c$& 0.24~$\pm$~0.02 & 17.93~$\pm$~0.03 & $-$18.43~$\pm$~0.03 & $-$1.20~$\pm$~0.06 & $-$0.12~$\pm$~0.06 & 0.16~$\pm$~0.06  &  \nodata &
\nodata & \nodata \\
  $r=1.3$$\arcsec$$^c$   & 0.24~$\pm$~0.02 & 18.19~$\pm$~0.03 & $-$18.17~$\pm$~0.03 & $-$0.90~$\pm$~0.06 & $-$0.03~$\pm$~0.06 & 0.07~$\pm$~0.06  &  \nodata & 
\nodata & \nodata \\ 
  $r=2.3$$\arcsec$$^c$   & 0.24~$\pm$~0.02 & 17.89~$\pm$~0.03 & $-$18.47~$\pm$~0.03 & $-$1.19~$\pm$~0.06 & $-$0.05~$\pm$~0.06 & 0.15~$\pm$~0.06  &  \nodata & 
\nodata & \nodata \\
  Tail & 0.24~$\pm$~0.02 & 20.59~$\pm$~0.05 & $-$15.77~$\pm$~0.05 & $-$0.40~$\pm$~0.20 &    0.28~$\pm$~0.09 & 0.30~$\pm$~0.06  &  \nodata & \nodata  & \nodata \\
\hline
\noalign{\smallskip}
{\bf SBS 1054+365}  & 0.02$^d$ & 15.46~$\pm$~0.03 & $-$14.06~$\pm$~0.03 & $-$0.34~$\pm$~0.06 &    0.33~$\pm$~0.06 & \nodata  &  0.92~$\pm$~0.08  & 
0.38~$\pm$~0.12  &   0.16~$\pm$~0.15  \\
  Main Body$^e$      & 0.02$^d$ & 15.83~$\pm$~0.03 & $-$13.69~$\pm$~0.03 & $-$0.45~$\pm$~0.06 &    0.23~$\pm$~0.06 & \nodata  &  0.72~$\pm$~0.08  &  \nodata 
&   \nodata        \\
  C$^c$       & 0.02$^d$ & 17.81~$\pm$~0.03 & $-$11.71~$\pm$~0.03 & $-$0.69~$\pm$~0.06 & $-$0.02~$\pm$~0.06 & \nodata  &  0.22~$\pm$~0.10  &  0.20:          & 
0.14:          \\
  a$^e$       & 0.02$^d$ & 18.81~$\pm$~0.03 & $-$10.71~$\pm$~0.03 & $-$0.52~$\pm$~0.06 &    0.19~$\pm$~0.06 & \nodata  &  0.50~$\pm$~0.12  &  \nodata        & 
\nodata        \\
  b$^c$       & 0.02$^d$ & 18.47~$\pm$~0.03 & $-$11.05~$\pm$~0.03 & $-$0.52~$\pm$~0.06 &    0.16~$\pm$~0.06 & \nodata  &  0.79~$\pm$~0.12  &  0.15:          &  
0.10:          \\
  d           & 0.02$^d$ & 19.97~$\pm$~0.03 &  $-$9.55~$\pm$~0.03 & $-$0.55~$\pm$~0.06 &    0.10~$\pm$~0.06 & \nodata  &  0.70~$\pm$~0.12  &  \nodata  & \nodata \\
  UC          & 0.02$^d$ & \nodata        &  \nodata	  &    0.11~$\pm$~0.08 &    0.42~$\pm$~0.08 & \nodata  &  1.05~$\pm$~0.15  &  0.7:  &  \nodata     \\
\noalign{\smallskip}
  Comp        & 0.02$^d$ & 16.84~$\pm$~0.03 &  \nodata	  & $-$0.10~$\pm$~0.06 &    0.61~$\pm$~0.06 & \nodata  &  \nodata	     &  \nodata        &  
\nodata        \\
  Comp~C$^f$& 0.02$^d$ & 17.42~$\pm$~0.03 &  \nodata	  & $-$0.28~$\pm$~0.06 &    0.49~$\pm$~0.06 & \nodata  &  1.75~$\pm$~0.08  &  0.66~$\pm$~0.10     & 
0.27~$\pm$~0.15  \\  
\hline
\noalign{\smallskip}
{\bf SBS 1211+540}$^c$& 0.08~$\pm$~0.01& 17.32~$\pm$~0.03&$-$13.27~$\pm$~0.03& $-$0.61~$\pm$~0.06&	 0.04~$\pm$~0.06 & 0.21~$\pm$~0.06  & \nodata & \nodata &
\nodata \\
  C$^c$	& 0.08~$\pm$~0.01 & 18.67~$\pm$~0.03 & $-$11.92~$\pm$~0.03 & $-$0.89~$\pm$~0.06 & $-$0.03~$\pm$~0.06 & 0.13~$\pm$~0.06  &  \nodata & \nodata & \nodata \\ 
  a$^c$	& 0.08~$\pm$~0.01 & 20.53~$\pm$~0.03 & $-$10.06~$\pm$~0.03 & $-$0.71~$\pm$~0.06 &	 0.00~$\pm$~0.06 & 0.15~$\pm$~0.06  &  \nodata & \nodata & \nodata \\
  b	    & 0.08~$\pm$~0.01 &  22.4~$\pm$~0.1  &   $-$8.2~$\pm$~0.1  &    \nodata 	    &	 0.45~$\pm$~0.15 & 0.48~$\pm$~0.10  &  \nodata & \nodata & \nodata \\
  UC    & 0.08~$\pm$~0.01 & \nodata        & \nodata           & $-$0.21~$\pm$~0.06 &	 0.29~$\pm$~0.06 & 0.35~$\pm$~0.06  &  \nodata & \nodata & \nodata \\
\hline
\noalign{\smallskip}
{\bf SBS 1319+579}  & 0.02~$\pm$~0.01 & 15.32~$\pm$~0.03 & $-$18.53~$\pm$~0.03 & $-$0.39~$\pm$~0.06 &    0.34~$\pm$~0.06 &    0.19~$\pm$~0.06 &  1.03~$\pm$~0.08 & 
0.39~$\pm$~0.12 &    0.16~$\pm$~0.20 \\
         A$^c$  & 0.02~$\pm$~0.01 & 17.61~$\pm$~0.03 & $-$16.24~$\pm$~0.03 & $-$0.77~$\pm$~0.06 & $-$0.04~$\pm$~0.06 &    0.02~$\pm$~0.06 &  0.31~$\pm$~0.12 & 
0.21~$\pm$~0.14 &         0.15~$\pm$~0.20 \\
         B$^c$  & 0.08~$\pm$~0.02 & 17.41~$\pm$~0.03 & $-$16.44~$\pm$~0.03 & $-$0.45~$\pm$~0.08 &    0.12~$\pm$~0.06 &    0.25~$\pm$~0.06 &  0.88~$\pm$~0.12 & 
0.28~$\pm$~0.16 &          \nodata\\
         C$^c$  & 0.02~$\pm$~0.01 & 17.98~$\pm$~0.03 & $-$15.87~$\pm$~0.03 & $-$0.72~$\pm$~0.06 &    0.02~$\pm$~0.06 &    0.12~$\pm$~0.06 &  0.68~$\pm$~0.12 & 
0.25~$\pm$~0.16 &          0.20: \\
            UC  & 0.02~$\pm$~0.01 &      \nodata   &         \nodata   & $-$0.15~$\pm$~0.08 &    0.29~$\pm$~0.06 &    0.33~$\pm$~0.06 &  1.20~$\pm$~0.20 &      \nodata &          \nodata\\
\hline
\noalign{\smallskip}
{\bf SBS 1415+437}  & 0.13~$\pm$~0.02 & 15.32~$\pm$~0.03 & $-$14.52~$\pm$~0.03 & $-$0.47~$\pm$~0.06 & 0.21~$\pm$~0.06 & 0.27~$\pm$~0.06 &  0.98~$\pm$~0.08 &  0.35~$\pm$~0.10 &    0.15: \\
             C  & 0.13~$\pm$~0.02 & 16.97~$\pm$~0.03 & $-$12.87~$\pm$~0.03 & $-$0.75~$\pm$~0.06 & 0.01~$\pm$~0.06 & 0.08~$\pm$~0.06 &  0.60~$\pm$~0.12 &  0.20~$\pm$~0.14 &    0.1:	\\
             a  & 0.13~$\pm$~0.02 & 19.04~$\pm$~0.03 & $-$10.80~$\pm$~0.03 & $-$0.68~$\pm$~0.06 & 0.06~$\pm$~0.06 & 0.12~$\pm$~0.06 &    \nodata     &    \nodata	  &    \nodata \\
             b  & 0.13~$\pm$~0.02 & 19.53~$\pm$~0.03 & $-$10.31~$\pm$~0.03 & $-$0.49~$\pm$~0.06 & 0.18~$\pm$~0.06 & 0.31~$\pm$~0.06 &    \nodata     &    \nodata	 &    \nodata \\
            UC  & 0.13~$\pm$~0.02 &      \nodata   & $-$     \nodata   & $-$0.17~$\pm$~0.08 & 0.27~$\pm$~0.06 & 0.38~$\pm$~0.06 &  1.10~$\pm$~0.14 &    \nodata	
&    \nodata \\
\noalign{\smallskip}
           bg  & 0.009$^b$      & 19.69~$\pm$~0.03 &         \nodata   &    0.33~$\pm$~0.08 & 1.35~$\pm$~0.06 & 0.88~$\pm$~0.06 &  1.22~$\pm$~0.12 &  0.55~$\pm$~0.14 &    \nodata  \\
\hline
{\bf III Zw 107}$^c$ & 0.21~$\pm$~0.02 & 14.36~$\pm$~0.03 & $-$20.14~$\pm$~0.03& $-$0.42~$\pm$~0.06 & 0.14~$\pm$~0.06 &  0.22~$\pm$~0.06 & 0.62~$\pm$~0.12 & 0.47~$\pm$~0.20 & 0.35~$\pm$~0.20 \\ 
A$^{c,d}$ & 0.47~$\pm$~0.02 & 15.67~$\pm$~0.03 & $-$18.83~$\pm$~0.03& $-$0.68~$\pm$~0.06 & $-$0.01~$\pm$~0.06&0.15~$\pm$~0.06 &  0.56~$\pm$~0.12 &   0.36~$\pm$~0.20 &    0.20~$\pm$~0.20 \\
B+C$^{c,d}$ & 0.11~$\pm$~0.02 & 15.75~$\pm$~0.03 & $-$18.75~$\pm$~0.03& $-$0.57~$\pm$~0.06 & 0.02~$\pm$~0.06 &  0.18~$\pm$~0.06 &  0.76~$\pm$~0.14 &  0.42~$\pm$~0.20
&    0.24~$\pm$~0.20 \\
Tail        & 0.21~$\pm$~0.02 & 18.66~$\pm$~0.03 & $-$15.84~$\pm$~0.03& $-$0.15~$\pm$~0.06 & 0.20~$\pm$~0.06 &  0.30~$\pm$~0.06 & \nodata & \nodata & \nodata \\
UC           & 0.21~$\pm$~0.02 & \nodata        & \nodata          &    0.06~$\pm$~0.10 & 0.40~$\pm$~0.08 &  0.30~$\pm$~0.08 & 1.2: & \nodata & \nodata \\
\hline
\noalign{\smallskip}
    {\bf Tol 9}$^c$  & 0.31~$\pm$~0.03 & 13.92~$\pm$~0.03 & $-$19.26~$\pm$~0.03 &  $-$0.34~$\pm$~0.06 &    0.24~$\pm$~0.06 &	 0.22~$\pm$~0.06 &  0.83~$\pm$~0.08 & 
0.68~$\pm$~0.10 &    0.27~$\pm$~0.12 \\
            UC  & 0.31~$\pm$~0.03 &  \nodata       &    \nodata        &     0.04~$\pm$~0.10 &    0.48~$\pm$~0.08 &	 0.33~$\pm$~0.08 &  1.10~$\pm$~0.20 & 
\nodata       &    \nodata       \\
\noalign{\smallskip}
          Comp 1 & 0.07$^b$      & 16.78~$\pm$~0.03 & $-$16.40~$\pm$~0.03 &     0.17~$\pm$~0.08 &    0.63~$\pm$~0.06 &	 0.39~$\pm$~0.06 &  1.15~$\pm$~0.10 & 
0.69~$\pm$~0.14 &    0.29~$\pm$~0.16 \\
          Comp 2 & 0.07$^b$      & 15.33~$\pm$~0.03 & $-$17.85~$\pm$~0.03 &     0.29~$\pm$~0.06 &    0.65~$\pm$~0.06 &	 0.52~$\pm$~0.06 &  1.55~$\pm$~0.10 & 
0.73~$\pm$~0.14 &    0.30~$\pm$~0.16 \\
\hline
\noalign{\smallskip}
{\bf Tol 1457-262} \\
     Obj 1$^c$  &  0.16$^b$  & 14.44~$\pm$~0.03 & $-$19.73~$\pm$~0.03 & $-$0.56~$\pm$~0.06 & 0.23~$\pm$~0.06 & 0.26~$\pm$~0.06 &  0.60~$\pm$~0.10 & 
0.51~$\pm$~0.12 &    0.22~$\pm$~0.12 \\
    	 A$^c$  &  0.57      & 14.47~$\pm$~0.03 & $-$19.70~$\pm$~0.03 & $-$0.80~$\pm$~0.06 & 0.08~$\pm$~0.06 & 0.11~$\pm$~0.06 &  0.30~$\pm$~0.12 & 
0.38~$\pm$~0.12 &    0.15~$\pm$~0.12 \\
    	 B$^c$  &  0.16$^b$  & 16.31~$\pm$~0.03 & $-$17.86~$\pm$~0.03 & $-$0.63~$\pm$~0.06 & 0.13~$\pm$~0.06 & 0.16~$\pm$~0.06 &  0.40~$\pm$~0.12 & 
0.35~$\pm$~0.12 &    0.19~$\pm$~0.14 \\
    	 C$^c$  &  0.16$^b$  & 17.63~$\pm$~0.03 & $-$16.54~$\pm$~0.03 & $-$0.58~$\pm$~0.06 & 0.26~$\pm$~0.06 & 0.21~$\pm$~0.06 &  \nodata  &  \nodata  &  \nodata	  \\
    	 d$^c$  &  0.16$^b$  & 17.21~$\pm$~0.03 & $-$16.96~$\pm$~0.03 & $-$0.49~$\pm$~0.06 & 0.19~$\pm$~0.06 & 0.11~$\pm$~0.06 &  0.60~$\pm$~0.16 & \nodata &  \nodata \\
      UC  &  0.16$^b$  & \nodata        & \nodata      	  & $-$0.30~$\pm$~0.14 & 0.31~$\pm$~0.12 & 0.32~$\pm$~0.08 &  1.20~$\pm$~0.20 &  \nodata & \nodata \\
\noalign{\smallskip}
     Obj 2$^c$  &  0.16$^b$  & 15.20~$\pm$~0.03 & $-$18.97~$\pm$~0.03 & $-$0.42~$\pm$~0.06 & 0.34~$\pm$~0.06 & 0.36~$\pm$~0.06 &  0.90~$\pm$~0.10 & 
0.58~$\pm$~0.12 &    0.27~$\pm$~0.14 \\
   	 e$^c$  &  0.16$^b$  & 17.17~$\pm$~0.03 & $-$17.00~$\pm$~0.03 & $-$0.61~$\pm$~0.06 & 0.27~$\pm$~0.06 & 0.36~$\pm$~0.06 &  1.10~$\pm$~0.20 &  \nodata       & 
\nodata   \\
   	 f$^c$  &  0.16$^b$  & 16.81~$\pm$~0.03 & $-$17.36~$\pm$~0.03 & $-$0.53~$\pm$~0.06 & 0.37~$\pm$~0.06 & 0.33~$\pm$~0.06 &  1.30~$\pm$~0.20 &  \nodata       & 
\nodata   \\
   	 g$^c$  &  0.16$^b$  & 15.93~$\pm$~0.03 & $-$18.24~$\pm$~0.03 & $-$0.30~$\pm$~0.06 & 0.44~$\pm$~0.06 & 0.41~$\pm$~0.06 &  1.20~$\pm$~0.20 &  \nodata       &  
\nodata   \\
            UC  &  0.16$^b$  & \nodata        & \nodata      	  & $-$0.17~$\pm$~0.14 & 0.45~$\pm$~0.12 & 0.53~$\pm$~0.08 &  1.30~$\pm$~0.20 &  \nodata  
&    \nodata       \\
\noalign{\smallskip}
          \#15  &  0.16$^b$  & 17.69~$\pm$~0.04 & $-$16.48~$\pm$~0.04 & $-$0.25~$\pm$~0.10 & 0.39~$\pm$~0.08 & 0.39~$\pm$~0.06 &  1.10~$\pm$~0.20 &  \nodata      
&    \nodata       \\
          \#16  &  0.16$^b$  & 19.48~$\pm$~0.05 & $-$14.69~$\pm$~0.05 & $-$0.10~$\pm$~0.15 & 0.45~$\pm$~0.10 & 0.40~$\pm$~0.06 &  \nodata       &  \nodata    
&    \nodata       \\
\hline
\noalign{\smallskip}
{\bf Arp 252}$^d$ \\
\noalign{\smallskip}
  A  & 0.34~$\pm$~0.02 & 14.69~$\pm$~0.03 & $-$20.88~$\pm$~0.03 & $-$0.48~$\pm$~0.06 & 0.31~$\pm$~0.06 & 0.19~$\pm$~0.06 &  1.10~$\pm$~0.10 &  0.60~$\pm$~0.12 &  
0.38~$\pm$~0.14$^e$ \\
 Aa1$^c$  & 0.34~$\pm$~0.02 & 15.27~$\pm$~0.03 & $-$20.30~$\pm$~0.03 & $-$0.67~$\pm$~0.06 & 0.08~$\pm$~0.06 & 0.14~$\pm$~0.06 &  0.95~$\pm$~0.10 &  0.48~$\pm$~0.12 & 
\nodata \\
 Aa2  & 0.34~$\pm$~0.02 & 17.77~$\pm$~0.03 & $-$17.80~$\pm$~0.03 & $-$0.50~$\pm$~0.06 & 0.12~$\pm$~0.06 & 0.17~$\pm$~0.06 &  1.10~$\pm$~0.20 &      \nodata   &	 
\nodata   \\
   c  & 0.34~$\pm$~0.02 & 19.89~$\pm$~0.04 & $-$15.58~$\pm$~0.04 & $-$0.75~$\pm$~0.09 & 0.03~$\pm$~0.07 & 0.08~$\pm$~0.06 &      \nodata   &      \nodata   &	 
\nodata   \\
  At  & 0.34~$\pm$~0.02 & \nodata        &    \nodata        &    \nodata       & 0.26~$\pm$~0.08 & 0.24~$\pm$~0.07 &      \nodata   &      \nodata   &	 
\nodata   \\
\hline
B  & 0.16~$\pm$~0.03 & 16.22~$\pm$~0.03 & $-$19.35~$\pm$~0.03 & $-$0.21~$\pm$~0.08 & 0.49~$\pm$~0.06 & 0.31~$\pm$~0.06 &  1.20~$\pm$~0.10 &  0.71~$\pm$~0.16 &  
0.34~$\pm$~0.20$^e$ \\
Bcen$^c$  & 0.16~$\pm$~0.03 & 16.51~$\pm$~0.03 & $-$19.06~$\pm$~0.03 & $-$0.41~$\pm$~0.06 & 0.38~$\pm$~0.06 & 0.30~$\pm$~0.06 &  1.00~$\pm$~0.10 &  0.52~$\pm$~0.12 &  
\nodata \\
d  & 0.16~$\pm$~0.03 & 21.65~$\pm$~0.05 & $-$13.92~$\pm$~0.05 & $-$0.35~$\pm$~0.12 & 0.23~$\pm$~0.10 & 0.10~$\pm$~0.08 &      \nodata   &      \nodata   &	 
\nodata   \\
e  & 0.16~$\pm$~0.03 & 19.45~$\pm$~0.04 & $-$16.12~$\pm$~0.04 & $-$0.31~$\pm$~0.09 & 0.27~$\pm$~0.07 & 0.20~$\pm$~0.06 &      \nodata   &      \nodata   &	 
\nodata   \\
BtN  & 0.16~$\pm$~0.03 & 17.22~$\pm$~0.04 & $-$18.35~$\pm$~0.04 &    0.05~$\pm$~0.10 & 0.43~$\pm$~0.08 & 0.29~$\pm$~0.06 &  1.30~$\pm$~0.20 &      \nodata   &	 
\nodata   \\
BtS  & 0.16~$\pm$~0.03 & \nodata        &    \nodata        &    0.20~$\pm$~0.12 & 0.53~$\pm$~0.08 & 0.39~$\pm$~0.06 &      \nodata   &      \nodata   &	 
\nodata   \\
\hline
\noalign{\smallskip}
{\bf NGC 5253}$^{c,d}$ & 0.17~$\pm$~0.03 & 10.09~$\pm$~0.01 & $-$17.92~$\pm$~0.01 & $-$0.41~$\pm$~0.02 & 0.27~$\pm$~0.02 & 0.21~$\pm$~0.02 & 0.81~$\pm$~0.03 & 0.53~$\pm$~0.04 & 0.19~$\pm$~0.05 \\
\hline
\end{tabular}} 
\par
%\smallskip
{\bf Notes for Table~5:}\\
  $^a$ Average value of the $E(B-V)$ obtained in objects/regions inside the galaxy. \\
  $^b$ Using the value for the Galactic extinction given by Schlegel et~al. (1998). \\
  $^c$ The optical colors of this object have been corrected for the emission of the ionized gas, consult Table~\ref{correccionemision2}.\\
  $^d$ Notes 1: {\bf HCG 31} See results in \citet{LSER04a}, member AC is NGC 1741. 
  {\bf Mkn 1087}: see results in \citet{LSER04b}. {\bf Haro 15}: using Cair\'os et~al. (2001a) data. {\bf Mkn 1199}: assuming a value similar to the near region B, that has not been analyzed by photometry but by spectroscopy. {\bf Mkn 5}: the colors of this object should be also corrected for emission of the gas, but as we do not have spectroscopic data it was not done. $B-V$ should be slightly lower and $V-R$ slightly higher. {\bf IRAS 08339+6517}: results extracted from \citet{LSEGR06}.  {\bf POX~4}: using the $E(B-V)$ derived for the central object. {\bf UM 420}: The \Ha\ emission in this object is very important; correcting for our \Ha\ flux $(V-R)\sim 0.25$. {\bf SBS 0926+606 X}: the $B$-magnitude of this object is very uncertain. Its $V$ and $K_{\rm s}$ magnitudes are $m_V$~=~22.1~$\pm$~0.1 and $m_{K_{\rm s}}=15.91$~$\pm$~0.12, hence it possesses $V-K_{\rm s}\sim6.2$. {\bf SBS 0948+532}: using the values given by 2MASS, $m_J=16.86$, $m_H=15.92$ and $m_{K_{\rm s}}=15.31$. {\bf SBS 1054+365}: because of the $C$(\Hb) derived from our spectrum gives $E(B-V)=0.01$, we use the Galactic value, $E(B-V)_G = 0.02$ (Schlegel et~al. 1998). {\bf III Zw 107}: using the data for $J$, $H$ and $K_{\rm s}$ provided by 2MASS. {\bf Arp 252}: object A is ESO 566-8 and object B ESO 566-7. {\bf NGC 5253}: optical and \NIR\ magnitudes extracted from the \NED\ and corrected for extinction using an average value of $C$(\Hb)~=~0.24 (see L\'opez-S\'anchez et~al. 2007).\\
  $^e$ NOTES 2: {\bf Mkn 5}: using the data provided by \citet{Noeske05}, who used $K'$ instead of $K_{\rm s}$ filter. For the low-brightness underlying stellar component, they found $J-H=0.58$ y $H-K'=0.28$. {\bf IRAS 08339+6517:} \NIR\ values extracted from 2MASS, see \citet{LSEGR06}. {\bf UM 420 / UGC 1809}: calculated using $V_{\rm r}=7306$~km~s$^{-1}$ (given by the \NED) and its derived distance, $D=97.4$~Mpc. {\bf SBS 1054+365}: probably, the colors have a small contribution for the nebular component. {\bf Arp 252:} $H-K_{\rm s}$ color adapted from 2MASS.\\
  $^f$ NOTES 3:  {\bf SBS 1054+365}: Comp C is the central region of the companion object, 2MASX J10574661+3616582.
\par
  \end{table}