\begin{table}%ta.11 online
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\par
\caption{\label{sbs1054lineas}Dereddened line intensity ratios with respect to $I$(\Hb)~=~100 for regions analyzed in SBS~0948+532, SBS~1054+365, and SBS~1211+540.}
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 {\small \begin{tabular}{l  r@{\hspace{5pt}}  r@{\hspace{8pt}}    r@{\hspace{8pt}}r@{\hspace{8pt}}r@{\hspace{8pt}}  }
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Line  & $f(\lambda)$&  SBS 0948+532    & SBS 1054+365 & SBS 1054+365 b & SBS 1211+540 \\
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 \tableline
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 3697.15    H	 I  &  0.262 &       0.48:   &        \nodata	&	   \nodata  &	     \nodata\\
 3703.86    H	 I  &  0.260 &  1.96  $\pm$  0.38	&	 \nodata   &	   \nodata  &	     \nodata\\
 3711.97    H	 I  &  0.259 &  1.25  $\pm$  0.32	&	 \nodata   &	   \nodata  &	     \nodata\\
 3721.83   [S III]  &  0.257 &  1.57  $\pm$  0.35	&	 \nodata   &	   \nodata  &	     \nodata\\
 3726.03   [O  II]  &  0.257 &  45.4  $\pm$  2.7   &	\nodata   &	   \nodata  &  33.0  $\pm$  3.8\\ 
 3728.00   [O  II]  &  0.256 &        \nodata	& 100.2  $\pm$  7.5   &	350  $\pm$  95  &	     \nodata\\
 3728.82   [O  II]  &  0.256 &  65.7  $\pm$  3.8   &	\nodata   &	   \nodata  &  44.8  $\pm$  4.6\\ 
 3734.17    H	 I  &  0.255 &  2.52  $\pm$  0.43	&	 \nodata   &	   \nodata  &	    2.61:\\   
 3750.15    H	 I  &  0.253 &  2.56  $\pm$  0.43	&	 \nodata   &	   \nodata  &	3.7  $\pm$  1.3\\ 
 3770.63    H	 I  &  0.249 &  2.88  $\pm$  0.45	&	1.53:	&	   \nodata  &	3.2  $\pm$  1.2\\ 
 3797.90    H	 I  &  0.244 &  5.11  $\pm$  0.71	&	2.85:	&	   \nodata  &	    3.99:\\   
 3819.61   He	 I  &  0.240 &  0.65  $\pm$  0.25	&	 \nodata   &	   \nodata  &	     \nodata\\
 3835.39    H	 I  &  0.237 &  7.74  $\pm$  0.77	&   6.8  $\pm$  1.3   &	   \nodata  &	5.9  $\pm$  1.5\\ 
 3868.75  [Ne III]  &  0.230 &  41.6  $\pm$  2.6   &  49.6  $\pm$  4.8   &	   \nodata  &  37.6  $\pm$  4.0\\ 
 3889.05    H	 I  &  0.226 &  19.7  $\pm$  1.5   &  19.8  $\pm$  2.8   &	   \nodata  &  19.9  $\pm$  3.0\\ 
 3967.46  [Ne III]  &  0.210 &  15.0  $\pm$  1.2   &  27.4  $\pm$  2.8   &	   \nodata  &  13.3  $\pm$  2.1\\ 
 3970.07    H	 I  &  0.210 &  16.2  $\pm$  1.2   &	\nodata   &	   \nodata  &  16.1  $\pm$  2.2\\ 
 4026.21   He	 I  &  0.198 &  1.45  $\pm$  0.32	&	 \nodata   &	   \nodata  &	     \nodata\\
 4068.60   [S  II]  &  0.189 &  1.53  $\pm$  0.33	&	2.05:	&	 \nodata    &	     \nodata\\
 4101.74    H	 I  &  0.182 &  26.2  $\pm$  1.7   &  26.4  $\pm$  3.0   &	  \nodata   &  26.2  $\pm$  3.0\\ 
 4340.47    H	 I  &  0.127 &  47.2  $\pm$  2.9   &  47.2  $\pm$  4.1   &	28.51:      &  47.3  $\pm$  4.1\\ 
 4363.21   [O III]  &  0.121 &  8.13  $\pm$  0.82	&   9.7  $\pm$  1.5   &	   \nodata  &  12.2  $\pm$  1.8\\ 
 4471.48   He	 I  &  0.095 &  3.81  $\pm$  0.49	&  3.31  $\pm$  0.81   &	   \nodata  &	4.6  $\pm$  1.3\\ 
 4658.10  [Fe III]  &  0.050 &       1.13:   &        \nodata	&	 \nodata    &	     \nodata\\
 4686.00   He	II  &  0.043 &  1.3  $\pm$  0.3	&  0.61  $\pm$  0.23   &	   \nodata  &	     \nodata\\
 4711.37  [Ar  IV]  &  0.037 &  0.85  $\pm$  0.25	&	1.18:	&	 \nodata    &	     \nodata\\
 4713.14   He	 I  &  0.037 &        \nodata	&	 \nodata   & \nodata	    &	    0.75:\\   
 4733.93  [Fe III]  &  0.031 &       0.18:   &        \nodata	&	 \nodata    &	     \nodata\\
 4740.16  [Ar  IV]  &  0.030 &  0.61  $\pm$  0.24   &        \nodata	&	 \nodata    &	    0.98:\\   
 4754.83  [Fe III]  &  0.026 &       0.34:   &        \nodata	&	 \nodata    &	     \nodata\\
 4861.33    H	 I  &  0.000 & 100.0  $\pm$  5.2   & 100.0  $\pm$  7.4   &   100  $\pm$  39     & 100.0  $\pm$  7.5\\ 
 4958.91   [O III]  & --0.024 & 189.5  $\pm$  9.2   &   210  $\pm$  13	&    75  $\pm$  23      &	163  $\pm$  10\\  
 4985.90  [Fe III]  & --0.031 &  1.49  $\pm$  0.30	&	 \nodata   &	   \nodata  &	     \nodata\\
 5006.84   [O III]  & --0.036 &   584  $\pm$  28   &   623  $\pm$  37   &   183  $\pm$  53	    &	481  $\pm$  29\\  
 5015.68   He	 I  & --0.038 &        \nodata	&	 \nodata   &   \nodata      &	    2.24:\\   
 5197.90   [N	I]  & --0.082 &        \nodata	&	1.03:	&	 \nodata    &	     \nodata\\
 5517.71  [Cl III]  & --0.154 &       0.39:   &        \nodata	&	 \nodata    &	     \nodata\\
 5537.88  [Cl III]  & --0.158 &       0.24:   &        \nodata	&	 \nodata    &	     \nodata\\
 5875.64   He	 I  & --0.215 & 10.76  $\pm$  0.81	&   8.7  $\pm$  1.6   &	   \nodata  &	     \nodata\\
 6300.30   [O	I]  & --0.282 &  3.00  $\pm$  0.31	&	1.12:	&	 \nodata    &	    2.36:\\   
 6312.10   [S III]  & --0.283 &  1.74  $\pm$  0.24	&	1.36:	&	 \nodata    &	2.8  $\pm$  1.1\\ 
 6363.78   [O	I]  & --0.291 &  1.07  $\pm$  0.23	&	0.65:	&	 \nodata    &	    0.57:\\   
 6548.03   [N  II]  & --0.318 &  2.45  $\pm$  0.30	&  2.02  $\pm$  0.74   &	  7.66:    &	    0.82:\\   
 6562.82    H	 I  & --0.320 &   278  $\pm$  14     &   277  $\pm$  17   &   279  $\pm$  74	    &	280  $\pm$  17\\  
 6583.41   [N  II]  & --0.323 &  6.21  $\pm$  0.60	&   5.6  $\pm$  1.0   &	 20.2:     &  2.24  $\pm$  0.89\\
 6678.15   He	 I  & --0.336 &  2.81  $\pm$  0.36	&  2.94  $\pm$  0.96   &	  7.40:    &	3.6  $\pm$  1.1\\ 
 6716.47   [S  II]  & --0.342 &        \nodata	&  10.1  $\pm$  1.2   &	    22.4:     &  5.65  $\pm$  0.88\\
 6730.85   [S  II]  & --0.344 &        \nodata	&  7.03  $\pm$  0.97   &	 19.6:    &  4.91  $\pm$  0.82\\
 7065.28   He	 I  & --0.387 &        \nodata	&  2.08  $\pm$  0.83   &	  \nodata   &	     \nodata\\
 7135.78  [Ar III]  & --0.396 &        \nodata	&   8.8  $\pm$  1.5   &	  \nodata   &	     \nodata\\					\noalign{\smallskip}
 \tableline
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Aperture size (arcsec)   &         &   3.6 &    6.4 &    5.8 &     3.6 \\
Distance$^a$ (arcsec)&       &   0 &      0 &    17.8 &      0              \\
$F$(\Hb)$^b$          &         &   8.44  $\pm$    0.32 &	14.57  $\pm$    0.68 &	0.66  $\pm$    0.13 &    1.84  $\pm$    0.09 \\ 
$C$(\Hb)              &         &   0.35  $\pm$    0.03 &	 0.02  $\pm$    0.02 &	0.6  $\pm$    0.1   &    0.12  $\pm$    0.01 \\
$W_{\rm abs}$ (\AA)     &         &    0.3  $\pm$  0.1 & 0.8   $\pm$    0.1  &	0.3   $\pm$    0.1  &    1.3   $\pm$    0.1  \\ 
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$-W$(\Ha) (\AA) & &  788    $\pm$    43   & 422    $\pm$    27   & 32    $\pm$     8   &   705    $\pm$    45   \\ 
$-W$(\Hb) (\AA) & &  213    $\pm$    11   & 89    $\pm$     7   &  8    $\pm$     3   &   135    $\pm$    10   \\ 
$-W$(H$\gamma$) (\AA)& &   57    $\pm$  4   & 43    $\pm$     4   & 2    $\pm$     1   &    74    $\pm$     7   \\ 
$-W$([O III]) 5007 (\AA)&     &  689    $\pm$    34   &	567    $\pm$    35   & 12    $\pm$     3   & 618    $\pm$    38   \\ 
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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.
\end{table}