\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).}
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 {\small \begin{tabular}{l  r@{\hspace{3pt}}  rrrrr}
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\hline \hline
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&       &        \multicolumn{3}{c}{SBS 1319+579}  &       \multicolumn{2}{c}{SBS 1415+437} \\   
Line & $f(\lambda)$& A     &  B             &  C       &   C     &  A \\
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 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:\\
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 \tableline
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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 \\
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$-W$(\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 \\
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$^a$ 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.
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