\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}