\begin{table}%T9
%\centering
\par
\caption{Parameters for representative models in agreement with the IQ (IQ1-IQ4) and 
flare states (F1 and F2) observed towards Sgr~A*.
These models are plotted in Figs.~\ref{Fig:1NIRMIR} and~\ref{Fig:2NIRMIR}.
The NIR flux density contributions from the synchrotron and SSC 
part of the spectrum as well as the SSC X-ray flux density 
are listed (Cols.~2 to~4). 
In the following columns we list  the magnetic field strength $B$, 
observed cutoff frequency $\nu_{\rm m, obs}$ and flux density $S_{\rm m, obs}$ 
of the synchrotron spectrum, 
size $\theta$ of the source component and the spectral index $\alpha$ 
of the synchrotron component.
All models except IQ2 provide synchrotron emission for frequencies up to
$\nu_2 \sim200$~THz. We assume that the cutoff in the energy spectrum
of the relativistic electrons can be represented via an exponential
cutoff in the observed synchrotron spectrum proportional to
$\exp[-(\nu/\nu_0)^{0.5}]$ with the effective cutoff frequency $\nu_0$.
In the first column the NIR flux densities are given without (in brackets) and with
modulation by the exponential cutoff.
\label{tab:models}}
\begin{tabular}{ccccccccccc}
\hline\hline
model & $S_{\rm NIR}$ & $S_{\rm NIR}$ &  $S_{\rm X-ray}$& $B$     & $\nu$$_{\rm max,obs}$ & $S_{\rm max,obs}$ & size     & $\alpha$$_{\rm NIR/X-ray}$  &$c/\nu$$_{0}$ \\
ID & synchr.   &  SSC      &             &       &                   &               &          &                &        \\
  & (mJy)     &  (mJy)    &  (nJy)      & (G)   & (GHz)             &  (Jy)         &($\mu$as) &                 & ($\mu$m)       \\ \hline
IQ1      &
%no cutoff required cuts off in NIR
0.8   &  2.0  & $<$18   & 17 & 820          & 3.9          & 7.9     & 1.3 & --\\
IQ2   &
%nocutoff required cuts off at 3 THz
--     &  3.0  & $<$27   & 5  & 820          & 7.7          & 8.1     & 1.3 & --\\
IQ3   &
%no cutoff required cuts off in NIR
(25)1 &  0.1 & $<$17   & 80 & 1000         & 16.0         & 17.5     & 1.0  & 15\\
IQ4   &
%no cutoff required cuts off in NIR
2.0   &  0.02 & $<$15   & 38 & 1500         & 0.33         & 1.5     & 0.8 & --\\
F1    &
%cutoff at 0.75 NIR 5mu
(18) 6&  1.13 & 65      & 68 & 1640         & 11.5         & 8.5     & 1.1 & 5\\
F2      &
%cutoff at 0.18 NIR 20mu
%(73) 6&  0.3  & 240     & 59 & 1640         & 10.5         & 8.5     & 0.8 & 20\\
%F3      &
%cutoff at NIR 90mu
(300) 6&  0.1  & 230    & 100 & 1640         & 5.7         & 8.5     & 0.4 & 90 \\
%F4      &
%cutoff at  NIR 6mu
%(33) 6&  0.3  & 250     & 46 & 1850         & 3.9         & 4.4     & 0.8  & 6\\
\hline
\end{tabular}
\end{table}