\begin{table}%ta.15 online %\centering \par \caption{\label{iiizw107lineas}Dereddened line intensity ratios with respect to $I$(\Hb)~=~100 for knots analyzed in III~Zw~107 (regions A, B, and C) and Tol~9 (spectra obtained with \INTe\ and \NOTe).} %\centerline {\small \begin{tabular}{l r@{\hspace{10pt}} rrrr r} \noalign{\smallskip} \hline \hline \noalign{\smallskip} \noalign{\smallskip} Line & $f(\lambda)$ & III Zw 107 A & III Zw 107 B & III Zw 107 C & Tol 9 INT & Tol 9 NOT \\ \noalign{\smallskip} \tableline \noalign{\smallskip} 3554.42 He I & 0.283 & \nodata & \nodata & \nodata & 3.8 $\pm$ 1.4 & \nodata \\ 3728.00 [O II] & 0.256 & 213 $\pm$ 12 & 306 $\pm$ 23 & 20.32: & 142 $\pm$ 10 & 177 $\pm$ 27\\ 3770.63 H I & 0.249 & 1.00: & 0.54: & \nodata & 0.56: & \nodata \\ 3797.90 H I & 0.244 & 2.37: & \nodata & \nodata & 0.83: & \nodata \\ 3835.39 H I & 0.237 & 3.60 $\pm$ 0.95 & 1.69: & 5.02: & 1.94: & \nodata \\ 3868.75 [Ne III] & 0.230 & 23.3 $\pm$ 2.1 & 21.1 $\pm$ 4.0 & 20.64: & 10.9 $\pm$ 2.0 & 12.08:\\ 3889.05 H I & 0.226 & 12.6 $\pm$ 1.7 & 11.1 $\pm$ 4.2 & 8.84: & 6.9 $\pm$ 2.1 & \nodata \\ 3967.46 [NeIII]H7 & 0.210 & 17.1 $\pm$ 1.7 & 22.4 $\pm$ 2.9 & \nodata & 21.6 $\pm$ 1.9 & \nodata \\ 4068.60 [S II] & 0.189 & 2.26 $\pm$ 0.82 & 4.69: & \nodata & 3.3 $\pm$ 1.1 & \nodata \\ 4101.74 H I & 0.182 & 26.2 $\pm$ 1.8 & 26.1 $\pm$ 4.2 & 27.5 $\pm$ 6.5 & 25.3 $\pm$ 2.5 & 26.3 $\pm$ 4.0 \\ 4340.47 H I & 0.127 & 46.7 $\pm$ 2.8 & 46.9 $\pm$ 4.8 & 47.5 $\pm$ 7.9 & 45.8 $\pm$ 3.2 & 46.9 $\pm$ 5.8 \\ 4363.21 [O III] & 0.121 & 3.14 $\pm$ 0.67 & 1.97: & \nodata & 0.55: & \nodata \\ 4471.48 He I & 0.095 & 4.08 $\pm$ 0.75 & 3.40: & \nodata & 3.94 $\pm$ 0.65 & 3.96:\\ 4658.10 [Fe III] & 0.050 & 1.06: & \nodata & \nodata & 1.09: & \nodata \\ 4686.00 He II & 0.043 & \nodata & \nodata & \nodata & 0.33: & \nodata \\ 4814.55 [Fe II] & 0.012 & \nodata & \nodata & \nodata & 0.85: & \nodata \\ 4861.33 H I & 0.000 & 100.0 $\pm$ 5.3 & 100.0 $\pm$ 8.2 & 100 $\pm$ 15 & 100.0 $\pm$ 6.0 & 100 $\pm$ 10\\ 4921.93 He I & --0.015 & 0.42: & \nodata & \nodata & \nodata & \nodata \\ 4958.91 [O III] & --0.024 & 123.7 $\pm$ 6.5 & 99.5 $\pm$ 8.1 & 93 $\pm$ 14 & 78.3 $\pm$ 5.2 & 75.5 $\pm$ 9.1\\ 5006.84 [O III] & --0.036 & 375 $\pm$ 18 & 293 $\pm$ 19 & 257 $\pm$ 32 & 236 $\pm$ 13 & 225 $\pm$ 21 \\ % 5047.74 He I & -0.046 & \nodata & 0.75: & \nodata & \nodata & \nodata \\ % 5158.81 [Fe II] & -0.073 & 0.72: & 2.63: & \nodata & \nodata & \nodata \\ 5197.90 [N I] & --0.082 & 1.08: & 2.07: & \nodata & \nodata & \nodata \\ 5200.26 [N I] & --0.083 & 0.36: & \nodata & \nodata & 2.63 $\pm$ 0.78 & \nodata \\ 5517.71 [Cl III] & --0.154 & 0.22: & \nodata & \nodata & 0.57: & \nodata \\ 5537.88 [Cl III] & --0.158 & 0.20: & \nodata & \nodata & 0.64: & \nodata \\ 5754.64 [N II] & --0.198 & \nodata & \nodata & \nodata & 0.41: & \nodata \\ 5875.64 He I & --0.215 & 12.5 $\pm$ 1.1 & 13.1 $\pm$ 2.3 & 12.94: & 12.6 $\pm$ 1.4 & 16.3 $\pm$ 3.8 \\ 6300.30 [O I] & --0.282 & 4.56 $\pm$ 0.61 & 6.1 $\pm$ 2.0 & 7.57: & 7.78 $\pm$ 0.71& 7.32 $\pm$ 0.96\\ 6312.10 [S III] & --0.283 & 1.02 $\pm$ 0.23 & \nodata & \nodata & 0.66: & 0.66:\\ 6363.78 [O~I] & --0.291 & 1.55 $\pm$ 0.42 & 2.01: & 3.58: & 2.14 $\pm$ 0.59 & 2.30 $\pm$ 0.91\\ 6548.03 [N~II] & --0.318 & 9.98 $\pm$ 0.75 & 12.1 $\pm$ 1.4 & 13.6 $\pm$ 4.5 & 23.8 $\pm$ 1.8 & 24.3 $\pm$ 2.3 \\ 6562.82 H I & --0.320 & 282 $\pm$ 16 & 273 $\pm$ 18 & 280 $\pm$ 35 & 267 $\pm$ 18 & 284 $\pm$ 30\\ 6583.41 [N~II] & --0.323 & 28.7 $\pm$ 1.8 & 37.0 $\pm$ 3.2 & 41.4 $\pm$ 8.3 & 72.2 $\pm$ 4.9 & 82.1 $\pm$ 7.3\\ 6678.15 He~I & --0.336 & 3.17 $\pm$ 0.50 & 4.01: & \nodata & 3.16 $\pm$ 0.64 & 4.1 $\pm$ 1.3 \\ 6716.47 [S II] & --0.342 & 19.6 $\pm$ 1.3 & 36.4 $\pm$ 4.3 & 52.2 $\pm$ 8.7 & 37.0 $\pm$ 2.6 & 42.1 $\pm$ 3.9 \\ 6730.85 [S II] & --0.344 & 15.9 $\pm$ 1.1 & 27.5 $\pm$ 3.6 & 35.6 $\pm$ 6.9 & 29.8 $\pm$ 2.2 & 35.7 $\pm$ 3.4\\ 7065.28 He I & --0.387 & 2.27 $\pm$ 0.40 & \nodata & \nodata & 1.93 $\pm$ 0.51 & 2.41 $\pm$ 0.94\\ 7135.78 [Ar III] & --0.396 & 11.4 $\pm$ 0.9 & 9.4 $\pm$ 1.7 & \nodata & 10.5 $\pm$ 1.0 & 10.8 $\pm$ 1.5\\ 7318.39 [O II] & --0.418 & 2.12 $\pm$ 0.58 & \nodata & \nodata & 1.96: & 1.57 $\pm$ 0.43\\ 7329.66 [O II] & --0.420 & 2.48 $\pm$ 0.66 & \nodata & \nodata & 1.08: & 1.30 $\pm$ 0.34\\ 7751.10 [Ar III] & --0.467 & \nodata & \nodata & \nodata & \nodata & 2.68 $\pm$ 0.68 \\ \noalign{\smallskip} \tableline \noalign{\smallskip} Aperture size (arcsec) & & 7.2$\times$1 & 5.6$\times$1 & 5.2$\times$1 & 6.4$\times$1 & 3.8$\times$1 \\ Distance (arcsec)$^a$& & -- & 7.2 & 12.4 & -- & -- \\ $F$(\Hb)$^b$ & & 22.3 $\pm$ 0.8 & 8.6 $\pm$ 0.4 & 1.56 $\pm$ 0.14 & 23.4 $\pm$ 0.9 & 3.8$\times$0.3\\ $C$(\Hb) & & 0.68 $\pm$ 0.04 & 0.15 $\pm$ 0.02 & 0.22 $\pm$ 0.03 & 0.50 $\pm$ 0.05 & 0.40 $\pm$ 0.05\\ $W_{\rm abs}$ (\AA) & & 2.0 $\pm$ 0.3 & 1.30 $\pm$ 0.10 & 0.50 $\pm$ 0.10 & 7.5 $\pm$ 0.8 & 6.2 $\pm$ 0.6 \\ \noalign{\smallskip} $-W$(\Ha) (\AA) & & 306 $\pm$ 18 & 76 $\pm$ 5 & 30 $\pm$ 4 & 178 $\pm$ 12 & 186 $\pm$ 15 \\ $-W$(\Hb) (\AA) & & 44 $\pm$ 3 & 15 $\pm$ 2 & 4.7 $\pm$ 0.7 & 33 $\pm$ 2 & 17 $\pm$ 3 \\ $-W$(H$\gamma$) (\AA)& & 16.4 $\pm$ 1.0 & 5.5 $\pm$ 0.6 & 1.8 $\pm$ 0.3 & 12.3 $\pm$ 0.8 \\ $-W$([O III]) 5007 (\AA)& & 172 $\pm$ 8 & 41 $\pm$ 3 & 11.6 $\pm$ 1.5 & 77 $\pm$ 4 & 32 $\pm$ 4\\ \noalign{\smallskip} \tableline \end{tabular}} \medskip $^a$ Relative distance of the knot with respect to the main region in the galaxy; $^b$ in units of 10$^{-15}$~erg~s$^{-1}$~cm$^{-2}$ and not corrected for extinction. \end{table}