\begin{table}%T3
\caption{\label{emission}Spectral properties of emission-line dwarfs. }
\small%\centering
\par
\begin{tabular}{lcccccccccc}
\hline\hline\noalign{\smallskip}
 &  H$\beta$ & $[$O{\scriptsize~III}$]$ & $[$O{\scriptsize~III}$]$ & $[$N{\scriptsize~II}$]$ &  H$\alpha$  & $[$N{\scriptsize~II}$]$ & $[$S{\scriptsize~II}$]$ & $[$S{\scriptsize~II}$]$ &  SFR  & $12+\log$O/H \\
\multicolumn{1}{c}{\raisebox{1.5ex}[-1.5ex]{Galaxy}} & $\lambda$4861.3 & $\lambda$4958.9 & $\lambda$5006.8 & $\lambda$6548.1 & $\lambda$6562.8 & $\lambda$6583.4 & $\lambda$6717.0 & $\lambda$6731.3 & $M_{\odot}$~yr$^{-1}$ & [dex] \\
\noalign{\smallskip}\hline
N5846\_06 & 348.1 &  45.8  &  128.4  &  14.0  & 992.0 &  51.7  &  66.6  &  47.7 & 0.0064(3) & 8.2(1) \\
N5846\_07 & 619.6 & -- &  4.2 &  62.5  & 1765.9 &  173.7  &  107.2  &  81.3 & 0.0114(4) & 8.4(1) \\
N5846\_08 & -- & -- & -- &  7.7  & 51.0  &  7.2  &  12.5  & 8.0 & -- & 8.5(1) \\
N5846\_09 & 79.0  & -- &  18.9  &  3.1  & 225.1 &  8.5  &  21.4  &  16.5 & -- & 8.1(1) \\
N5846\_12 & 300.1 &  93.9  &  270.4  &  7.9  & 855.4 &  16.6  &  47.5  &  26.7 & 0.0055(3) & 7.8(2) \\
N5846\_14 & 409.9 &  71.9  &  212.0  &  10.1  & 1168.3 &  47.8  &  89.3  &  64.0 & 0.0075(4) & 8.1(2) \\
N5846\_15 & -- & -- & -- & -- & 24.2  & -- & -- & -- & -- &  -- \\
N5846\_17 & -- & -- & -- & -- & 46.7  &  9.1  &  6.5  & 6.8 & -- & 8.6(1) \\
N5846\_18 & -- & -- & -- & -- & 30.7  & -- &  7.7  & 7.4 & -- &  -- \\
N5846\_19 & 43.7  & -- &  19.3  &  8.6  & 124.6 &  14.0  &  21.3  &  12.3 & -- & 8.4(1) \\
N5846\_20 & 171.1 &  5.4 &  39.9  &  17.5  & 487.5 &  42.4  &  51.4  &  37.5 & -- & 8.4(1) \\
N5846\_27 & -- & -- & -- & -- & 38.8  & -- &  7.9  & -- & -- &  -- \\
N5846\_28 & 298.8 &  15.6  &  50.1  &  21.2  & 851.5 &  67.1  &  64.5  &  52.6 & 0.0055(3) & 8.3(1) \\
N5846\_33 & -- & -- & -- & -- & 29.7  & -- & -- & -- & -- &  -- \\
N5846\_38 & 103.8 &  12.1  &  40.8  &  8.6  & 295.8 &  20.5  &  16.2  &  14.4 & -- & 8.3(1) \\
N5846\_39 & 34.0  & -- &  10.4  & -- & 96.8  &  9.3  &  19.2  &  12.7 & -- & 8.4(1) \\
N5846\_40 & -- & -- & -- & -- & 42.8  & -- &  9.3  & 5.9 & -- &  -- \\
N5846\_41 & 2576.2 &  1222.0  &  3664.0  &  20.6  & 7342.2 &  68.1  &  182.0  &  127.8  & 0.0473(9) & 7.6(2) \\
N5846\_42 & 914.9 &  475.5  &  1385.0  &  10.9  & 2607.5 &  31.4  &  76.4  &  48.9 & 0.0168(5) & 7.7(2) \\
N5846\_46 & 223.7 &  15.3  &  43.8  &  16.6  & 637.6 &  51.7  &  53.9  &  43.1 & 0.0041(3) & 8.3(1) \\
N5846\_49 & 28.9  & -- &  8.7 & -- & 82.3  &  2.4  &  5.3  & 7.7 & -- & 8.0(1) \\
N5846\_50 & -- & -- & -- & -- & 32.2  & -- & -- & -- & -- &  -- \\
N5846\_51 & 62.6  &  8.9 &  38.8  &  8.6  & 178.4 &  15.8  &  24.5  &  20.9 & -- & 8.4(1) \\
N5846\_54 & 290.9 & -- &  45.4  &  31.4  & 829.2 &  89.8  &  75.4  &  57.6 & 0.0053(3) & 8.4(1) \\
N5846\_55 & 461.1 & -- &  17.9  &  47.0  & 1314.2 &  140.1  &  81.2  &  61.9 & 0.0085(4) & 8.4(1) \\
N5846\_56 & 40.6  & -- &  15.6  &  12.0  & 115.7 &  10.5  &  14.1  &  10.2 & -- & 8.3(1) \\
\hline
\end{tabular}
\tablefoot{Fluxes present the integrals of the fitted Gaussians and are given in units of
10$^{-17}$~erg~s$^{-1}$~cm$^{-2}$. H$\alpha$ and H$\beta$ fluxes have been corrected for extinction. Numbers in parentheses indicate errors of the
last significant digit.}
\end{table}