\begin{table}%t8 \caption{\label{gasamount}H$_\alpha$ luminosities.} \par %\centering \par \begin{tabular}{lccc} \hline \hline \noalign{\smallskip} Name & $L_{\rm H\alpha} / 10^{40}~[\rm erg~s^{-1}]$ & Line \\ $(1)$ & $(2)$ & $(3)$ \\ \hline 1C7 & 100 & O[II]3727 \\ 1C8 & 20 & H$\beta$ \\ 1C9 & 100 & O[II]3727 \\ 1C10 & 100 & H$\beta$ \\ 1F2 & 20 & H$\beta$ \\ 1F3 & 20 & H$\beta$ \\ 1F4 & 40 & H$\alpha$ \\ 1F5 & 100 & H$\alpha$ \\ 1F6 & 10 & H$\alpha$ \\ 1F7 & 600 & O[II]3727 \\ 1F10 & 20 & O[III]5007 \\ 2C3 & 10 & H$\beta$ \\ 2C5 & 10 & H$\beta$ \\ 2C6 & 30 & O[II]3727 \\ 2C7 & 20 & O[III]5007 \\ 2C8 & 9 & H$\alpha$ \\ 2F1 & 30 & H$\beta$ \\ 2F2 & 1 & O[II]3727 \\ 2F3 & 100 & O[II]3727 \\ 2F4 & 10 & O[II]3727 \\ 2F5 & 7 & O[II]3727 \\ 2F6 & 30 & H$\alpha$ \\ 2F9 & 9 & O[III]5007 \\ 2F10 & 100 & O[III]5007 \\ 2F11 & 9 & H$\alpha$ \\ 2F12 & 30 & O[II]3727 \\ 2F15\&16 & -- & O[II]3727 \\ 3C3 & 50 & H$\alpha$ \\ 3C4 & 30 & O[III]5007 \\ 3C5 & 20 & O[III]5007 \\ 3C6 & 9 & O[II]3727 \\ 3C7 & 15 & O[III]5007 \\ 3F3 & 2 & O[III]5007 \\ 3F6 & 30 & H$\alpha$ \\ 3F7 & 30 & H$\alpha$ \\ 3F8 & 40 & O[II]3727 \\ 3F9 & 30 & H$\alpha$ \\ 4C2 & 20 & O[II]3727 \\ 4C3 & 8 & O[II]3727 \\ 4F3 & 300 & O[II]3727 \\ 4F4 & 100 & O[III]5007 \\ 4F5 & 100 & O[II]3727 \\ 4F6 & 50 & O[II]3727 \\ 4F7 & 200 & O[II]3727 \\ 4F8 & 60 & O[III]5007 \\ 4F9 & 80 & O[III]5007 \\ 4F12 & 200 & O[II]3727 \\ 4F13 & 100 & O[III]5007 \\ NGC 0628 & 50 & \\ NGC 2976 & 3 & \\ NGC 3031 & 14 & \\ NGC 3049 & -- & \\ NGC 3184 & 15 & \\ NGC 3521 & 20 & \\ NGC 3621 & 60 & \\ NGC 3938 & 15 & \\ NGC 4236 & 4 & \\ NGC 4536 & 50 & \\ NGC 4569 & 20 & \\ NGC 4579 & 30 & \\ NGC 4625 & -- & \\ NGC 4725 & -- & \\ NGC 5055 & 30 & \\ NGC 5194 & 70 & \\ NGC 5713 & -- & \\ NGC 7331 & 50 & \\ \hline \end{tabular} \tablefoot {Column (1): galaxy ID; Col.~(2): H$_\alpha$~luminosity; Col.~(3): emission line that is used for calculating the H$_\alpha$~luminosity.\\ The errors in H$_\alpha$~luminosities are estimated to be ${\sim}50\%$ based on the width of the histograms in Fig.~\ref{fl_rat}.} \end{table}