\begin{table}%ta.13 online %\centering \par \caption{\label{a13}Dereddened line intensity ratios with respect to $I$(\Hb)~=~100 for knots analyzed in SBS~1319+579 (regions~A, B, and~C) and SBS~1415+457 (regions~C and~A).} %\centerline {\small \begin{tabular}{l r@{\hspace{3pt}} rrrrr} \noalign{\smallskip} \hline \hline \noalign{\smallskip} & & \multicolumn{3}{c}{SBS 1319+579} & \multicolumn{2}{c}{SBS 1415+437} \\ Line & $f(\lambda)$& A & B & C & C & A \\ \noalign{\smallskip} \tableline \noalign{\smallskip} 4340.47 H I & 0.127 & 47.2 $\pm$ 2.6 & 47.4 $\pm$ 4.6 & 47.4 $\pm$ 3.1 & 47.5 $\pm$ 2.8 & 47.4 $\pm$ 3.8\\ 4363.21 [O III] & 0.121 & 9.98 $\pm$ 0.62 & 4.2 $\pm$ 1.0 & 3.73 $\pm$ 0.64 & 7.11 $\pm$ 0.61 & 6.1 $\pm$ 1.2\\ 4387.93 He I & 0.115 & 0.43 $\pm$ 0.17 & \nodata & 1.12: & \nodata & \nodata\\ 4437.55 He I & 0.104 & 0.20: & \nodata & \nodata & \nodata & \nodata\\ 4471.48 He I & 0.095 & 3.85 $\pm$ 0.36 & 4.4 $\pm$ 1.6 & 3.88 $\pm$ 0.68 & 3.86 $\pm$ 0.49 & 2.80 $\pm$ 0.66\\ 4658.10 [Fe III] & 0.050 & \nodata & \nodata & 0.72: & 1.05 $\pm$ 0.32 & 0.99:\\ 4686.00 He II & 0.043 & 0.8: & \nodata & \nodata & 2.35 $\pm$ 0.23 & \nodata\\ 4711.37 [Ar IV] & 0.037 & 2.14 $\pm$ 0.35 & \nodata & \nodata & \nodata & \nodata\\ 4713.14 He I & 0.037 & \nodata & \nodata & \nodata & 0.30: & \nodata\\ 4740.16 [Ar IV] & 0.030 & 1.61 $\pm$ 0.26 & \nodata & \nodata & 0.56: & \nodata\\ 4861.33 H I & 0.000 & $100.0 \pm 4.9$ & $100.0 \pm 8.5$ & $100.0 \pm 6.2$ &$100.0 \pm 4.9$ & $100.0 \pm 6.3$ \\ 4881.00 [Fe III] & --0.005 & \nodata & \nodata & \nodata & 0.21: & \nodata\\ 4921.93 He I & --0.015 & 0.96 $\pm$ 0.23 & \nodata & 0.75: & 1.41 $\pm$ 0.33 & \nodata\\ 4958.91 [O III] & --0.024 & 232 $\pm$ 12 & 132 $\pm$ 10 & 129.9 $\pm$ 7.4 & 107.5 $\pm$ 5.5 & 107.3 $\pm$ 6.5\\ 4985.90 [Fe III] & --0.031 & \nodata & \nodata & \nodata & 1.35 $\pm$ 0.33 & 1.19:\\ 5006.84 [O III] & --0.036 & \nodata & \nodata & \nodata & 301 $\pm$ 14 & 286 $\pm$ 16\\ 5015.68 He I & --0.038 & \nodata & \nodata & \nodata & $1.52 \pm 0.34$ & \nodata\\ 5875.64 He I & --0.215 & $11.90 \pm 0.86$ & $11.7 \pm 3.2$ & $11.2 \pm 1.2$ & $9.61 \pm 0.92$ & $7.7 \pm 1.1$\\ 6300.30 [O I] & --0.282 & $1.74 \pm 0.26$ & 3.08:& $4.77\pm0.72$ & $3.44 \pm 0.43$ & $2.41 \pm 0.56$\\ 6312.10 [S III] & --0.283 & 1.56 $\pm$ 0.29 & 1.14: & 1.80 $\pm$ 0.52 & 1.34 $\pm$ 0.31 & 0.98:\\ 6363.78 [O I] & --0.291 & 0.60 $\pm$ 0.18 & 1.28: & 1.48 $\pm$ 0.52 & 0.96 $\pm$ 0.31 & 0.86:\\ 6548.03 [N II] & --0.318 & 1.44 $\pm$ 0.27 & 3.8 $\pm$ 1.5 & 5.50 $\pm$ 0.72 & 1.13 $\pm$ 0.35 & 1.07:\\ 6562.82 H I & --0.320 & 280 $\pm$ 13 & 279 $\pm$ 19 & 281 $\pm$ 15 & 274 $\pm$ 13 & 278 $\pm$ 17\\ 6583.41 [N II] & --0.323 & 4.08 $\pm$ 0.42 & 13.1 $\pm$ 2.4 & 14.8 $\pm$ 1.3 & 4.30 $\pm$ 0.45 & 3.49 $\pm$ 0.98\\ 6678.15 He I & --0.336 & 2.97 $\pm$ 0.34 & 2.7 $\pm$ 1.1 & 2.87 $\pm$ 0.66 & 2.31 $\pm$ 0.41 & 2.28 $\pm$ 0.66\\ 6716.47 [S II] & --0.342 & 7.79 $\pm$ 0.56 & 26.0 $\pm$ 3.2 & 27.9 $\pm$ 1.9 & 13.15 $\pm$ 0.83 & 9.2 $\pm$ 1.1\\ 6730.85 [S II] & --0.344 & 5.76 $\pm$ 0.44 & 17.8 $\pm$ 2.9 & 18.9 $\pm$ 1.3 & 9.60 $\pm$ 0.63 & 6.71 $\pm$ 0.94\\ 7065.28 He I & --0.387 & 2.69 $\pm$ 0.36 & \nodata & 2.09 $\pm$ 0.54 & 1.49 $\pm$ 0.34 & 2.09 $\pm$ 0.66\\ 7135.78 [Ar III] & --0.396 & 4.76 $\pm$ 0.47 & 6.6 $\pm$ 1.6 & 6.06 $\pm$ 0.72 & 3.77 $\pm$ 0.38 & 3.28 $\pm$ 0.61\\ 7281.35 He I & --0.414 & 0.62: & \nodata & \nodata & \nodata & \nodata\\ 7318.39 [O II] & --0.418 & 1.30 $\pm$ 0.23 & 3.1 $\pm$ 1.0 & 2.69 $\pm$ 0.33 & 2.05 $\pm$ 0.33 & 1.56 $\pm$ 0.62\\ 7329.66 [O II] & --0.420 & 1.17 $\pm$ 0.24 & 2.01: & 1.94 $\pm$ 0.27 & 1.73 $\pm$ 0.35 & 1.35:\\ 7751.10 [Ar III] & --0.467 & 1.55 $\pm$ 0.25 & \nodata & \nodata & 0.96 $\pm$ 0.31 & 0.94:\\ \noalign{\smallskip} \tableline \noalign{\smallskip} Aperture size (arcsec) & & $6 \times 1$ & $2.8 \times 1$ & $5.6 \times 1$ & $6 \times 1$ & $3.4 \times 1$\\ Distance (arcsec)$^a$& & -- & 10 & 29 & -- & 6 \\ $F$(\Hb)$^b$ & & 14.57 $\pm$ 0.53 & 1.97 $\pm$ 0.10 & 8.18 $\pm$ 0.32 & 18.51 $\pm$ 0.66 & 4.07 $\pm$ 0.17 \\ $C$(\Hb) & & 0.03 $\pm$ 0.01 & 0.11 $\pm$ 0.03 & 0.02 $\pm$ 0.02 & 0.01 $\pm$ 0.02 & 0.16 $\pm$ 0.03 \\ $W_{\rm abs}$ (\AA) & & 0.0 $\pm$ 0.1 & 0.4 $\pm$ 0.1 & 0.2 $\pm$ 0.1 & 0.8 $\pm$ 0.1 & 1.0 $\pm$ 0.2 \\ \noalign{\smallskip} $-W$(\Ha) (\AA) & & 1530 $\pm$ 75 & 162 $\pm$ 11 & 295 $\pm$ 23 & 1300 $\pm$ 65 & 1187 $\pm$ 75 \\ $-W$(\Hb) (\AA) & & 285 $\pm$ 14 & 42 $\pm$ 4 & 94 $\pm$ 6 & 222 $\pm$ 11 & 130 $\pm$ 8 \\ $-W$(H$\gamma$) (\AA)& & 84 $\pm$ 5 & 15 $\pm$ 1 & 23 $\pm$ 1 & 73 $\pm$ 4 & 58 $\pm$ 5 \\ %$-W$([O II]) (\AA) & & \nodata & \nodata & \nodata & \nodata & \nodata \\ %$-W$([O III]) 4959 (\AA)& & 622 $\pm$ 31 & 47 $\pm$ 4 & 79 $\pm$ 5 & 250 $\pm$ 13 & 289 $\pm$ 18 \\ $-W$([O III]) 5007~(\AA)& & \nodata & \nodata & \nodata & 542 $\pm$ 26 & 574 $\pm$ 32 \\ %$-W$([N II]) (\AA) & & 25 $\pm$ 3 & 7.7 $\pm$ 1.4 & 15 $\pm$ 1 & 14 $\pm$ 1 & 12 $\pm$ 3 \\ %$-W$([S II]) 6717 (\AA)& & 50 $\pm$ 4 & 16 $\pm$ 2 & 29 $\pm$ 2 & 49 $\pm$ 3 & 33 $\pm$ 4 \\ %$-W$([S II]) 6731 (\AA)& & 36 $\pm$ 2 & 12 $\pm$ 2 & 25 $\pm$ 2 & 35 $\pm$ 2 & 17 $\pm$ 2 \\ \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}