\begin{table}%t8
\caption{\label{abundances}Emission lines used to measure abundances of the host galaxies of SNe~2007bg and~2007bi.}
%\centering
\small
\begin{tabular}{l l l}
\hline\hline \noalign{\smallskip}
Emission line	& SN 2007bg & SN 2007bi \\
\hline
$[$O {\scriptsize II}$]$ $\lambda3727$ 	&  $-$						& 3.75 $\pm$ 0.93 \\
H$\beta$ $\lambda4861$ 					& 6.19 $\pm$ 0.69 	& 1.20 $\pm$ 0.45 \\
$[$O {\scriptsize III}$]$ $\lambda4959$ & 8.45 $\pm$ 0.71 	& 1.75 $\pm$ 0.95 \\
$[$O {\scriptsize III}$]$ $\lambda5007$ & 17.81 $\pm$ 1.82 	& 3.53 $\pm$ 1.07 \\
H$\alpha$ $\lambda6563$ 				& 16.01 $\pm$ 1.62 	& 3.33 $\pm$ 0.84 \\
$[$N {\scriptsize II}$]$ $\lambda6584$ 	& 0.91 $\pm$ 0.13 	& ${<}0.43$ \\
\hline
\end{tabular}
\tablefoot {Emission line fluxes in units 10$^{-17}$~erg~s$^{-1}$~cm$^2$. Errors quoted are the uncertainties measured when fitting Gaussian profiles to the emission lines of the host galaxies. For the host of SN~2007bi an additional component is included in the errors to account for the uncertainty of subtracting off the SN~continuum (set~at a conservative~20\% of the measured line flux).}
\end{table}