\begin{table}
%\caption{Star formation rates derived from \ha\ and $I$ flux} \label{sfrs}
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%\begin{tabular}{rrrrrrrr} \hline \hline
%ID & \cal{F}$_{\rm H\alpha}$ & L$_{\rm H\alpha}$ & SFR & \cal{F}$_I$ & L$_{\rm uv}$ & SFR & R \\
%(1) & (2) & (3) & (4) & (5) & (6) & (7) & (8) \\ \hline
%  5 &   2.5 &   2.0 &   16 &  14.8 &  37.1 &   52 &   0.3 \\
% 79 &   1.9 &   1.5 &   11 &   9.4 &  23.4 &   33 &   0.4 \\
%131 &   4.2 &   3.3 &   26 &   5.4 &  13.5 &   19 &   1.4 \\
%132 &  23.3 &  18.2 &  144 &  43.0 & 107.6 &  151 &   1.0 \\
%144 &  20.7 &  16.2 &  128 &  38.2 &  95.5 &  134 &   1.0 \\
%152 &   0.9 &   0.7 &    5 &   1.3 &   3.3 &    5 &   1.2 \\
%176 &  10.4 &   8.1 &   64 &  38.2 &  95.7 &  134 &   0.5 \\
%183 &   3.9 &   3.0 &   24 &  11.5 &  28.7 &   40 &   0.6 \\
%$^a$199 &  85.3 &  66.8 &  528 &  58.8 & 147.2 &  206 &   2.6 \\
%207 &   1.3 &   1.1 &    8 &   3.5 &   8.8 &   12 &   0.7 \\
%211 &   5.5 &   4.3 &   34 &  23.3 &  58.3 &   82 &   0.4 \\
%212 &   1.1 &   0.9 &    7 &   3.0 &   7.5 &   10 &   0.7 \\
%215 &  12.1 &   9.5 &   75 &  61.8 & 154.6 &  216 &   0.3 \\
%229 &  82.0 &  64.2 &  507 &  88.8 & 222.2 &  311 &   1.6 \\
%269 &  33.0 &  25.8 &  204 &  65.0 & 162.5 &  228 &   0.9 \\
%329 &   1.6 &   1.2 &   10 &   1.9 &   4.9 &    7 &   1.4 \\
%388 &   1.0 &   0.8 &    6 &   1.8 &   4.5 &    6 &   1.0 \\
%457 &   2.0 &   1.6 &   13 &   4.0 &  10.1 &   14 &   0.9 \\
%477 &   2.0 &   1.6 &   13 &   6.5 &  16.4 &   23 &   0.5 \\ 
%\hline \hline
%\end{tabular}
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%\footnotesize \noindent Notes: (1) Number in catalogue based on
%NB~2.07 image (2) Continuum subtracted narrow band flux density in
%$10^{-19}$ erg cm $^{-2}$ s$^{-1}$ \AA$^{-1}$ (3) Corresponding
%luminosity at $z = 2.16$ in $10^{42}$ erg s$^{-1}$ corrected for a
%25\% [\ion{N}{II}] contribution (4) Corresponding star formation rate
%in M$_\odot$ yr$^{-1}$ (5) $I$ band flux density in $10^{-19}$ erg cm
%$^{-2}$ s$^{-1}$ \AA$^{-1}$ (6) Corresponding luminosity at $z = 2.16$
%in $10^{28}$ erg s$^{-1}$ Hz$^{-1}$ at rest frame wavelength of $\sim$
%2500 \AA\ (7) Corresponding star formation rate in M$_\odot$
%yr$^{-1}$ (8) Ratio of SFR(H$\alpha$) / SFR(uv) (a) Radio galaxy \rg
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\par
%\end{table}