\begin{table}%T8
%\centering
\par
\caption{Emission properties of the radio flare events from Sgr~A*.
In the case of a flare event detection we 
we give the estimated peak flux density,
the full zero start and stop times, the full zero width 
at the corresponding zero points (FWZP) and the full width at half maximum of the flare events. 
For the VLA we give the excess flux density over the mean flux density 
measured on 06 and 08 July.
\label{RADIOobs}}
\begin{tabular}{cccccccc}
\hline\hline
Observing & IR Flare & $\lambda$    & Start              & Stop            & FWZP  & {\it FWHM} & peak flux     \\
ID  & ID   &              &                    &                 & (min) & (min)& (Jy)          \\
\hline
SMA-A  & SMA1& 890~$\mu$m &    05 Jul. 07:00 &      05 Jul. 10:30 & 210   & 120   &       3.5       \\
SMA-A  & SMA2& 890~$\mu$m &    05 Jul. 11:00 & $\ge$05 Jul. 12:10 & --     & --     &  $\ge$3.2       \\
SMA-B  & SMA3& 890~$\mu$m &    06 Jul. 07:45 &      06 Jul. 10:00 & 135   & $<$60 &       3.4       \\
SMA-C  & SMA4& 890~$\mu$m &$<$07 Jul. 06:00 &      07 Jul. 08:00 &  --    & --     &  $\ge$3.5       \\
SMA-C  & SMA5& 890~$\mu$m &    07 Jul. 08:00 & $\ge$07 Jul. 12:00 &  --    & --     &       3.3       \\
VLA-B  & VLA1& 7~mm        &$<$07 Jul. 04:40 & $>$07 Jul. 08:50 &       &       &    $>$0.5       \\
\hline
\end{tabular}
\end{table}