\begin{table}%T1
%\centering
\par
\caption{Source widths (half intensity) and flux density of the flare emission at $\sim$11:10 UT (extended phase). Note the significantly larger diameter at the higher frequency.}
\label{table_sunmap_data}
\begin{tabular}{lllll}
   \hline\hline Frequency & Beamwidth & $\Theta_{{\rm meas}}$ & $\Theta_{{\rm source}}$ & Flux density \\[-1mm]
   [GHz] & [arcsec] & [arcsec] & [arcsec] & [sfu] \\
   \hline 230 & $117\pm 7$ & 124 & $42\pm20$ & $112^{+5}_{-4}$ \\
   345 & $88\pm 5$ & 112 & $70\pm6$ & 196$^{+14}_{-9}$ \\
   \hline 
\end{tabular}
\end{table}