\begin{table}%ta.15 online
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\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).}
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Line &   $f(\lambda)$ & III Zw 107 A &  III Zw 107 B &  III Zw 107 C  & Tol 9 INT &   Tol 9 NOT \\
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 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 \\
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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 \\ 
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$-W$(\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\\ 
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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}