\begin{table}%t4
\caption{Reddening-corrected fluxes for all \ion{H}{ii}~regions in the Sculptor group dwarfs.}\label{tabcap:Reddening-corrected-fluxes-for}
\small%\centerline
 {
\begin{tabular}{rccccccccc}
\hline
\hline 
 & AM106-382  & ESO~245-G005  & ESO 245-G005  & ESO 347-G017  & ESO~473-G024  & NGC 59  & NGC 59  & NGC 625  & NGC 625\\
Ion~~ $\lambda$ {[}\AA]  &  & external  & central  &  &  & \#1  & \#2  & \#1  & \#2\\
\hline 
{[}\ion{O}{ii}] 3726.0  & 2.007 $\pm$ 0.041  & 1.508 $\pm$ 0.018  & 2.767 $\pm$ 0.087  & 2.191 $\pm$ 0.016  & 0.942 $\pm$ 0.023  & 1.080 $\pm$ 0.029  & 2.716 $\pm$ 0.092  & 1.454 $\pm$ 0.019  & 1.516 $\pm$ 0.009 \\
H11 3770.6  & \ldots{}  & \ldots{}  & \ldots{}  & \ldots{}  & \ldots{}  & \ldots{}  & \ldots{}  & 0.049 $\pm$ 0.016  & 0.052 $\pm$ 0.008 \\
H10 3797.9  & \ldots{}  & \ldots{}  & \ldots{}  & \ldots{}  & \ldots{}  & \ldots{}  & 0.622 $\pm$ 0.086  & 0.064 $\pm$ 0.016  & 0.063 $\pm$ 0.008 \\
\ion{He}{i} 3819.6  & 0.143 $\pm$ 0.037  & \ldots{}  & \ldots{}  & \ldots{}  & \ldots{}  & \ldots{}  & 0.424 $\pm$ 0.084  & \ldots{}  & \ldots{} \\
H9 3835.4  & \ldots{}  & \ldots{}  & \ldots{}  & \ldots{}  & \ldots{}  & \ldots{}  & \ldots{}  & 0.085 $\pm$ 0.016  & 0.077 $\pm$ 0.008 \\
{[}\ion{Ne}{iii}] 3868.8  & 0.513 $\pm$ 0.037  & 0.146 $\pm$ 0.016  & 0.312 $\pm$ 0.071  & 0.348 $\pm$ 0.015  & 0.190 $\pm$ 0.021  & 0.374 $\pm$ 0.026  & 0.932 $\pm$ 0.082  & 0.274 $\pm$ 0.015  & 0.207 $\pm$ 0.008 \\
{[}\ion{Ne}{iii}]+H8 3879.0  & \ldots{}  & \ldots{}  & \ldots{}  & \ldots{}  & \ldots{}  & \ldots{}  & \ldots{}  & \ldots{}  & \ldots{} \\
H8 3889.1  & \ldots{}  & 0.151 $\pm$ 0.016  & 0.160 $\pm$ 0.070  & 0.117 $\pm$ 0.014  & 0.155 $\pm$ 0.020  & 0.217 $\pm$ 0.026  & \ldots{}  & 0.247 $\pm$ 0.015  & 0.186 $\pm$ 0.008 \\
H$\epsilon$ 3970.1  & \ldots{}  & 0.138 $\pm$ 0.014  & 0.209 $\pm$ 0.066  & 0.163 $\pm$ 0.013  & 0.209 $\pm$ 0.018  & 0.250 $\pm$ 0.023  & \ldots{}  & 0.258 $\pm$ 0.015  & 0.208 $\pm$ 0.007 \\
\ion{He}{i} 4026.2  & \ldots{}  & \ldots{}  & \ldots{}  & \ldots{}  & \ldots{}  & \ldots{}  & \ldots{}  & 0.024 $\pm$ 0.013  & \ldots{} \\
{[}\ion{S}{ii}]blend 4072.0  & \ldots{}  & \ldots{}  & \ldots{}  & \ldots{}  & \ldots{}  & \ldots{}  & \ldots{}  & \ldots{}  & \ldots{} \\
H$\delta$ 4101.7  & \ldots{}  & 0.212 $\pm$ 0.013  & 0.183 $\pm$ 0.057  & 0.172 $\pm$ 0.011  & 0.235 $\pm$ 0.016  & 0.250 $\pm$ 0.020  & \ldots{}  & 0.265 $\pm$ 0.013  & 0.248 $\pm$ 0.006 \\
H$\gamma$ 4340.5  & 0.518 $\pm$ 0.032  & 0.442 $\pm$ 0.010  & 0.483 $\pm$ 0.042  & 0.438 $\pm$ 0.010  & 0.401 $\pm$ 0.012  & 0.466 $\pm$ 0.020  & 0.481 $\pm$ 0.047  & 0.465 $\pm$ 0.010  & 0.463 $\pm$ 0.005 \\
{[}\ion{O}{iii}] 4363.2  & \ldots{}  & 0.032 $\pm$ 0.010  & 0.055 $\pm$ 0.037  & 0.049 $\pm$ 0.009  & 0.045 $\pm$ 0.011  & 0.038 $\pm$ 0.020  & 0.063 $\pm$ 0.045  & 0.028 $\pm$ 0.010  & 0.017 $\pm$ 0.004 \\
\ion{He}{i} 4471.5  & \ldots{}  & \ldots{}  & \ldots{}  & \ldots{}  & 0.027 $\pm$ 0.008  & 0.033 $\pm$ 0.013  & \ldots{}  & 0.035 $\pm$ 0.008  & 0.046 $\pm$ 0.004 \\
H$\beta$ 4861.3  & 1.000 $\pm$ 0.024  & 1.000 $\pm$ 0.008  & 1.000 $\pm$ 0.034  & 1.000 $\pm$ 0.009  & 1.000 $\pm$ 0.007  & 1.000 $\pm$ 0.014  & 1.000 $\pm$ 0.042  & 1.000 $\pm$ 0.009  & 1.000 $\pm$ 0.005 \\
{[}\ion{O}{iii}] 4958.9  & 0.616 $\pm$ 0.020  & 0.588 $\pm$ 0.007  & 1.072 $\pm$ 0.036  & 1.267 $\pm$ 0.009  & 0.786 $\pm$ 0.006  & 1.629 $\pm$ 0.016  & 1.337 $\pm$ 0.052  & 1.421 $\pm$ 0.010  & 1.089 $\pm$ 0.005 \\
{[}\ion{O}{iii}] 5006.8  & 1.782 $\pm$ 0.024  & 1.797 $\pm$ 0.010  & 3.223 $\pm$ 0.058  & 3.849 $\pm$ 0.013  & 2.473 $\pm$ 0.011  & 4.883 $\pm$ 0.023  & 2.930 $\pm$ 0.057  & 4.268 $\pm$ 0.017  & 3.304 $\pm$ 0.008 \\
{[}\ion{Fe}{iii}] 5412.0  & \ldots{}  & 0.034 $\pm$ 0.008  & \ldots{}  & \ldots{}  & \ldots{}  & \ldots{}  & \ldots{}  & \ldots{}  & \ldots{} \\
\ion{He}{i} 5875.7  & 0.159 $\pm$ 0.030  & 0.082 $\pm$ 0.012  & 0.104 $\pm$ 0.045  & 0.095 $\pm$ 0.011  & 0.062 $\pm$ 0.012  & 0.106 $\pm$ 0.019  & 0.152 $\pm$ 0.056  & 0.106 $\pm$ 0.011  & 0.093 $\pm$ 0.006 \\
{[}\ion{S}{iii}] 6312.1  & \ldots{}  & 0.047 $\pm$ 0.014  & \ldots{}  & \ldots{}  & \ldots{}  & 0.039 $\pm$ 0.023  & \ldots{}  & 0.049 $\pm$ 0.012  & \ldots{} \\
{[}\ion{O}{i}] 6363.8  & \ldots{}  & \ldots{}  & \ldots{}  & \ldots{}  & \ldots{}  & \ldots{}  & \ldots{}  & 0.006 $\pm$ 0.013  & \ldots{} \\
H$\alpha$ 6562.8  & 2.850 $\pm$ 0.043  & 2.594 $\pm$ 0.024  & 2.849 $\pm$ 0.103  & 2.592 $\pm$ 0.020  & 2.849 $\pm$ 0.037  & 2.850 $\pm$ 0.032  & 2.850 $\pm$ 0.090  & 2.850 $\pm$ 0.020  & 2.850 $\pm$ 0.011 \\
{[}\ion{N}{ii}] 6583.4  & \ldots{}  & \ldots{}  & 0.069 $\pm$ 0.103  & 0.064 $\pm$ 0.020  & 0.029 $\pm$ 0.037  & 0.075 $\pm$ 0.032  & \ldots{}  & \ldots{}  & \ldots{} \\
\ion{He}{i} 6678.1  & \ldots{}  & \ldots{}  & \ldots{}  & 0.016 $\pm$ 0.016  & 0.033 $\pm$ 0.017  & 0.023 $\pm$ 0.025  & 0.031 $\pm$ 0.064  & 0.029 $\pm$ 0.015  & 0.030 $\pm$ 0.009 \\
{[}\ion{S}{ii}] 6716.5  & 0.125 $\pm$ 0.040  & 0.134 $\pm$ 0.018  & 0.265 $\pm$ 0.068  & 0.208 $\pm$ 0.016  & 0.089 $\pm$ 0.019  & 0.129 $\pm$ 0.025  & 0.282 $\pm$ 0.064  & 0.130 $\pm$ 0.015  & 0.139 $\pm$ 0.009 \\
{[}\ion{S}{ii}] 6730.8  & 0.045 $\pm$ 0.040  & 0.114 $\pm$ 0.018  & 0.164 $\pm$ 0.068  & 0.144 $\pm$ 0.017  & 0.058 $\pm$ 0.019  & 0.105 $\pm$ 0.025  & 0.318 $\pm$ 0.065  & 0.123 $\pm$ 0.015  & 0.097 $\pm$ 0.009 \\
\ion{He}{i} 7065.3  & \ldots{}  & \ldots{}  & \ldots{}  & 0.021 $\pm$ 0.018  & \ldots{}  & 0.027 $\pm$ 0.028  & \ldots{}  & 0.027 $\pm$ 0.017  & 0.026 $\pm$ 0.011 \\
{[}\ion{Ar}{iii}] 7135.8  & \ldots{}  & \ldots{}  & \ldots{}  & 0.070 $\pm$ 0.019  & \ldots{}  & 0.105 $\pm$ 0.029  & 0.137 $\pm$ 0.075  & 0.110 $\pm$ 0.018  & 0.098 $\pm$ 0.011 \\
{[}\ion{O}{ii}]blend 7325.0  & \ldots{}  & \ldots{}  & \ldots{}  & \ldots{}  & \ldots{}  & \ldots{}  & \ldots{}  & \ldots{}  & \ldots{} \\
C H$\alpha$/H$\beta$$^{a}$  & 0.002 $\pm$ 0.042  & 0.000 $\pm$ 0.019  & 0.192 $\pm$ 0.076  & 0.192 $\pm$ 0.076  & 0.191 $\pm$ 0.022  & 0.017 $\pm$ 0.028  & 0.302 $\pm$ 0.079  & 0.042 $\pm$ 0.018  & 0.004 $\pm$ 0.010 \\
\hline
\end{tabular}}
\medskip
Notes: $^{a}$ The reddening constant is computed by the expression:
$I_{{\rm H}\alpha}/I_{{\rm H}\beta}=I_{{\rm H}\alpha0}/I_{{\rm H}\beta0}10^{-C[f({\rm H}\alpha)-f({\rm H}\beta)]}$, where $I_{0}$ and $I$ denote the flux before and after extinction,
and $f(\lambda)$ is the extinction curve.
\end{table}