\begin{table}%ta.1 online
\caption{\label{haro15lineas}Dereddened line intensity ratios with respect to $I$(\Hb)~=~100 for knots analyzed in Haro~15.}
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 {\small   \begin{tabular}{l  r rrr r}
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Line  & $f(\lambda)$&  $C$  &  $A$  &  $B$  & $D$\\
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 \tableline 
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 3705.04   He    I &   0.260 &       1.05:   &        \nodata   &        \nodata&        \nodata\\
 3728.00   [O  II] &   0.256 &   $294\pm19$   & $113\pm21$   &        $402\pm106$ & $336\pm46$\\ 
 3770.63    H    I &   0.249 &       0.68:   &  $1.69\pm0.52$   &        \nodata&        \nodata\\
 3797.90    H    I &   0.244 &       0.33:   &  $3.10\pm1.00$  &        \nodata&        \nodata\\
 3835.39    H    I &   0.237 &       1.69:   &  $4.59\pm0.99$   &        \nodata&        \nodata\\
 3868.75  [Ne III] &   0.230 &  $14.2\pm2.8$   &  $48.6\pm8.4$   &        \nodata& 39.4:\\
 3889.05    H    I &   0.226 &   $7.6\pm3.0$   &  $15.5\pm2.8$   &        \nodata&        \nodata\\
 3967.46  [Ne III] &   0.210 &        \nodata   &  $29.6\pm4.8$   &        \nodata&        \nodata\\
 3970.07    H    I &   0.210 &  $19.6\pm1.7$   &        \nodata   &        \nodata&        \nodata\\
 4026.21   He    I &   0.198 &        \nodata   &  1.05:   &        \nodata&        \nodata\\
 4068.60   [S  II] &   0.189 &       2.69:   &        \nodata   &        \nodata&        \nodata\\
 4101.74    H    I &   0.182 &  $28.1\pm2.7$   &  $26.1\pm3.5$   &        \nodata &$26.1\pm7.0$\\
 4340.47    H    I &   0.127 &  $46.2\pm3.5$   &  $47.0\pm4.8$   &        \nodata & $46.7 \pm 9.9$\\
 4363.21   [O III] &   0.121 &       1.22:   &  $8.59\pm0.87$   &        \nodata&3.9:\\
 4471.48   He    I &   0.095 &       3.56:   &  $4.17\pm0.68$   &        \nodata&        \nodata\\
 4658.10  [Fe III] &   0.050 &       1.75:   &       0.90:   &        \nodata&        \nodata\\
 4686.00   He   II &   0.043 &       0.49:   &  $1.65\pm0.42$   &        \nodata&        \nodata\\
 4711.37  [Ar  IV] &   0.037 &        \nodata   &  1.10:   &        \nodata&        \nodata\\
 4740.16  [Ar  IV] &   0.030 &        \nodata   &  0.73:   &        \nodata&        \nodata\\
 4754.83  [Fe III] &   0.026 &        \nodata   &       0.25:   &        \nodata&        \nodata\\
 4861.33    H    I &   0.000 & $100.0\pm6.7$   & $100.0\pm5.9$   &   $100\pm39$ & $100\pm19$\\
 4921.93   He    I &  --0.015 &        \nodata   &       0.55:   &        \nodata&        \nodata\\
 4958.91   [O III] &  --0.024 &  $67.2\pm5.0$   &   $212\pm11$   &    $81\pm30$&  $132 \pm 19$ \\
 5006.84   [O III] &  --0.036 &   $210\pm13$   &   $648\pm36$   &   $232\pm63$ & $383\pm44$\\
 5015.68   He    I &  --0.038 &       1.02:   &        \nodata   &        \nodata&        \nodata\\
 5158.81  [Fe  II] &  --0.073 &       1.95:   &        \nodata   &        \nodata&        \nodata\\
 5197.90   [N   I] &  --0.082 &       2.76:   &        \nodata   &        \nodata&        \nodata\\
 5517.71  [Cl III] &  --0.154 &        \nodata   &       0.33:   &        \nodata&        \nodata\\
 5537.88  [Cl III] &  --0.158 &        \nodata   &       0.26:   &        \nodata&        \nodata\\
 5875.64   He    I &  --0.215 &  $12.8\pm1.6$   &  $9.95\pm1.70$   &      46.1:& $10.5\pm2.8$\\
 6300.30   [O   I] &  --0.282 &   $7.5\pm1.1$   &  $2.21\pm0.76$   &        \nodata& $7.7 \pm 3.1$ \\
 6312.10   [S III] &  --0.283 &       1.10:   &  $1.16\pm0.31$   &        \nodata&        \nodata\\
 6363.78   [O   I] &  --0.291 &       2.18:   &     0.65:   &        \nodata&        \nodata\\
 6548.03   [N  II] &  --0.318 &  $20.1\pm1.8$   &  $2.82\pm0.71$   &        \nodata&6.0:\\
 6562.82    H    I &  --0.320 &   $288\pm19$   &   $202\pm46$   &   $284\pm75$& $288 \pm 35$ \\
 6583.41   [N  II] &  --0.323 &  $64.8\pm4.6$   &  $7.76\pm1.84$   &      23.4:& $23.2\pm6.1$\\
 6678.15   He    I &  --0.336 &       2.81:   &  $2.55\pm0.74$   &        \nodata& 3.9:\\
 6730.85   [S  II] &  --0.344 &  $18.0\pm2.0$   &  $5.09\pm1.32$   &      28.5:& $17.6\pm8.3$ \\
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 \tableline
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Aperture size (arcsec)       &   &    $6 \times 1$ &  $8.4 \times 1$  &  $8 \times 1$ & $4.4 \times 1$ \\
Distance$^b$ (arcsec)   &   &       0 &     13 &  23                  &  12  \\
$F$(\Hb)$^a$          &   &  $23.25 \pm   1.08$ &   $23.42 \pm   0.89$ &    $0.52 \pm   0.10$ & $1.32 \pm 0.12$ \\ 
$C$(\Hb)              &   &  $ 0.11 \pm   0.03$ &    $0.33 \pm   0.03$ &    $0.06 \pm   0.03$ & $0.37 \pm 0.02$\\
$W_{\rm abs}$ (\AA)     &   &    $2.4 \pm    0.4$ &     $1.3 \pm   0.3$  &    0.5               & $2.2 \pm 0.2$\\            
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$-W$(\Ha) (\AA)         &   &   $75.2 \pm    5.0$ &   $423.6 \pm   22.5$ &    $43.9 \pm   10.0$ & $48.8 \pm 2.7$\\ 
$-W$(\Hb) (\AA)         &   &   $16.4 \pm    1.1$ &    $75.7 \pm    4.2$ &     $8.4 \pm    3.2$ & $20.8 \pm 1.3$ \\ 
$-W$(H$\gamma$) (\AA)   &   &    $5.5 \pm    0.4$ &    $26.9 \pm    1.5$ &     \nodata          &  $7.5 \pm 0.9$  \\ 
$-W$([O III]) 5007~(\AA)&   &   $29.4 \pm 1.8$ &   $462.7 \pm  23.1$ &    $20.2 \pm    5.1$ & $77.9 \pm 3.9$ \\ 
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$^a$ In units of 10$^{-15}$~erg~s$^{-1}$~cm$^{-2}$ and not corrected for extinction; $^b$~relative distance with respect to the center of Haro~15.
\end{table}