\begin{table}%t3
\caption{\label{Table:Linesflux1}Reddening-corrected line ratios, normalized to \Hb\tablefootmark{*} for the
  sample of galaxies.}
\small%\centering
\par
\begin{tabular}{llcccccccccc}       
\hline\hline\noalign{\smallskip}
$\lambda$  & Ion  & \multicolumn{4}{c}{Mrk 407} &                                   
                    \multicolumn{6}{c}{Mrk 32} \\    
           &      & \multicolumn{2}{c}{Nuclear} & 
	            \multicolumn{2}{c}{Integrated}  & % mrk407
                    \multicolumn{2}{c}{Knot AB} & 
		    \multicolumn{2}{c}{Knot C} & 
		    \multicolumn{2}{c}{Integrated} \\ %mrk32
           &      & $F_{\lambda}$  &  $-W_{\lambda}$  & 
	            $F_{\lambda}$  &  $-W_{\lambda}$  & 
		    $F_{\lambda}$  &  $-W_{\lambda}$  &
                    $F_{\lambda}$  &  $-W_{\lambda}$  & 
		    $F_{\lambda}$  &  $-W_{\lambda}$  \\  
\hline
3727 &  [\ion{O}{ii}]    &  
                      $4.53\pm0.54$  &   $ 43.8\pm 3.3$   &   
		      $4.95\pm1.22$  &   $ 49.9\pm10.3$   &  
                      $3.21\pm0.31$  &   $ 34.9\pm 1.8$   &   
		      $4.77\pm0.56$  &   $ 33.9\pm 2.6$   &   
		      $4.76\pm0.71$  &   $ 26.9\pm 2.4$   \\  
3869 &  [\ion{Ne}{iii}]  & 
                      --            &   --              &   
		      --            &   --              &   
                      $0.44\pm0.08$  &   $  6.8\pm 1.2$   &   
		      --            &   --              &   
		      --            &   --              \\  
3889 &  H8+HeI      & 
                      --            &   --              &   
		      --            &   --              &   
                      --            &   --              &   
		      --            &   --              &   
		      --            &   --              \\  
3968 &  [\ion{Ne}{iii}]  & 
                      --            &   --              &   
		      --            &   --              &   
                      --            &   --              &   
		      --            &   --              &   
		      --            &   --              \\  
4101 & H$\delta$         &  
                      --            &   --              &   
		      --            &   --              &   
                      $0.25\pm0.03$  &   $  4.1\pm0.4$    &   
		      --            &   --              &   
		      --            &   --              \\  
4340 & H$\gamma$         &  
                      $0.27\pm0.05$  &   $  2.4\pm0.4$    &   
		      --            &   --              &   
                      $0.48\pm0.04$  &   $  9.3\pm0.6$    &   
		      $0.47\pm0.04$  &   $  4.6\pm0.3$    &   
		      $0.52\pm0.08$  &   $  4.0\pm0.5$    \\  
4363 & [\ion{O}{iii}]    & 
                      --            &   --              &   
		      --            &   --              &   
                      $0.08\pm0.02$  &   $  1.5\pm0.5$    &   
		      --            &   --              &   
		      --            &   --              \\  
4471 &  \ion{He}{i}      &
                      --            &   --              &   
		      --            &   --              &   
                      --            &   --              &   
		      --            &   --              &   
		      --	     &   --              \\  
4861 & H$\beta$          &  
                      $1.00\pm0.00$  &   $ 10.5\pm0.3$    &   
		      $1.00\pm0.00$  &   $ 10.2\pm0.7$    &   
                      $1.00\pm0.00$  &   $ 24.2\pm0.7$    &   
		      $1.00\pm0.00$  &   $ 11.7\pm0.4$    &   
		      $1.00\pm0.00$  &   $  9.8\pm0.6$    \\  
4959 & [\ion{O}{iii}]    & 
                      $1.17\pm0.06$  &   $ 12.8\pm0.4$    &    
		      $1.04\pm0.12$  &   $ 10.1\pm0.9$    &   
                      $0.99\pm0.04$  &   $ 25.8\pm0.7$    &   
		      $0.90\pm0.06$  &   $ 11.6\pm0.5$    &   
		      $0.87\pm0.09$  &   $  9.2\pm0.7$    \\  
5007 &  [\ion{O}{iii}]   & 
                      $3.16\pm0.13$  &   $ 35.3\pm0.4$    &   
		      $2.70\pm0.23$  &   $ 26.2\pm0.9$    &   
                      $2.82\pm0.11$  &   $ 70.8\pm0.8$    &   
		      $2.53\pm0.12$  &   $ 33.0\pm0.6$    &   
		      $2.20\pm0.16$  &   $ 23.2\pm0.7$    \\  
5876 &  \ion{He}{i}      & 
                      --            &   --              &   
		      --            &   --              &   
                      $0.12\pm0.02$  &   $  4.0\pm0.6$    &   
		      $0.16\pm0.03$  &   $  2.7\pm0.6$    &   
		      --            &   --              \\  
6300 &  [\ion{O}{i}]    & 
                      --            &   --              &    
		      --            &   --              &   
                      $0.09\pm0.01$  &   $  3.4\pm0.5$    &   
		      $0.10\pm0.02$  &   $  1.9\pm0.4$    &   
		      $0.15\pm0.02$  &   $  2.4\pm0.3$    \\ 
6548 &  [\ion{N}{ii}]    & 
                      --            &   --              &   
		      --            &   --              &   
                      --            &   --              &   
		      --            &   --              &   
		      --            &   --              \\  
6563 & H$\alpha$        & 
                      $2.86\pm0.16$  &   $ 53.0\pm0.4$    &   
		      $2.86\pm0.32$  &   $ 46.6\pm0.9$    &   
                      $2.87\pm0.12$  &   $107.4\pm1.4$    &   
		      $2.86\pm0.18$  &   $ 63.9\pm0.7$    &   
		      $2.86\pm0.26$  &   $ 46.4\pm0.7$    \\  
6584 &  [\ion{N}{ii}]    & 
                      $0.26\pm0.02$  &   $  4.8\pm0.3$    &   
		      $0.23\pm0.04$  &   $  3.7\pm0.6$    &   
                      $0.14\pm0.02$  &   $  5.4\pm0.9$    &   
		      $0.23\pm0.03$  &   $  5.1\pm0.7$    &   
		      $0.21\pm0.04$  &   $  3.4\pm0.7$    \\  
6678 &  \ion{He}{i}      &
                      $0.04\pm0.01$  &   $  0.8\pm0.2$    &  % mrk 407 nuclear 
		      --            &   --              &  % mrk 407 Integrated
                      --            &   --              &  % mrk 32  knotAB 
		      --            &   --              &  % mrk 32  knotC 
		      --            &   --              \\ % mrk 32  Integrated
6717 & [\ion{S}{ii}]     & 
                      $0.31\pm0.02$  &   $  6.0\pm0.3$    &  % mrk 407 nuclear 
		      $0.37\pm0.06$  &   $  6.2\pm0.7$    &  % mrk 407 Integrated
                      $0.38\pm0.02$  &   $ 15.7\pm0.5$    &  % mrk 32  knotAB 
		      $0.33\pm0.03$  &   $  6.9\pm0.4$    &  % mrk 32  knotC  
		      $0.49\pm0.06$  &   $  8.4\pm0.6$    \\ % mrk 32  Integrated
6731 & [\ion{S}{ii}]     & 
                      $0.25\pm0.02$  &   $  4.9\pm0.3$    &  % mrk 407 nuclear 
		      $0.30\pm0.05$  &   $  5.2\pm0.7$    &  % mrk 407 Integrated
                      $0.29\pm0.02$  &   $ 11.7\pm0.5$    &  % mrk 32  knotAB 
		      $0.26\pm0.03$  &   $  5.4\pm0.5$    &  % mrk 32  knotC  
		      $0.39\pm0.05$  &   $  6.5\pm0.6$    \\ % mrk 32  Integrated
      &          &  
                    \multicolumn{2}{c}{$F(\Hb)=336.3\pm 45.8 $} &  
                    \multicolumn{2}{c}{$F(\Hb)=408.4\pm110.9 $} &  
                    \multicolumn{2}{c}{ $F(\Hb)=113.4\pm  6.6 $} &  
                    \multicolumn{2}{c}{ $F(\Hb)= 24.4\pm  3.8 $} &  % mrk32 knot2 == brote C
                    \multicolumn{2}{c}{$F(\Hb)=232.6\pm 52.6 $} \\ % mrk32 int
     &          &              
		    \multicolumn{2}{c}{$\CHbeta=0.237\pm0.057 $} &  % mrk407 nucl
                    \multicolumn{2}{c}{$\CHbeta=0.165\pm0.113 $} &  % mrk407 int
                    \multicolumn{2}{c}{ $\CHbeta=0.108\pm0.021 $} &  % mrk32 knot1 == brote AB
                    \multicolumn{2}{c}{ $\CHbeta=0.167\pm0.065 $} &  % mrk32 knot2 == brote C
                    \multicolumn{2}{c}{$\CHbeta=0.107\pm0.095 $} \\ % mrk32 int
     &          &	    
                    \multicolumn{2}{c}{$\EBV=0.163\pm0.039$}  &  % mrk407 nucl
                    \multicolumn{2}{c}{$\EBV=0.114\pm0.078$}  &  % mrk407 int
                    \multicolumn{2}{c}{ $\EBV=0.075\pm0.014$}  &  % mrk32 knot1 == brote AB
                    \multicolumn{2}{c}{ $\EBV=0.115\pm0.045$}  &  % mrk32 knot2 == brote C
                    \multicolumn{2}{c}{$\EBV=0.074\pm0.065$}  \\ % mrk32 int
\hline
\end{tabular}
\tablefoot{\tablefoottext{*}{Reddening-corrected line fluxes, normalized to $F(\Hb)=1$. 
Equivalent widths of Balmer lines are corrected for underlying stellar 
absorption. The reddening coefficient, $\CHbeta$, \EBV\  
(derived as $0.69\times\CHbeta$) and the reddening-corrected \Hb\ flux, 
$F(\Hb) (\times 10^{-16}$~erg~cm$^{-2}$~s$^{-1}$) are listed for each 
region. 
The quoted uncertainties account for measurement, flux-calibration and 
reddening coefficient errors.}} 
\end{table}