\begin{table}%t4
\caption{Summary of the observed fluxes and errors of the \uchii~region G268.42-0.85.
As the error of the NIR~photometry, we give the statistical error of the PSF fit.
The last but one column indicates if the given flux density was included in the
SED fitting (see Sect.~\ref{SEDdiscussion}).
Notes: $^a$ PSF-Fit; $^b$ filter centered on Br~$\alpha$; $^c$ narrow-band filter; $^d$ flux standard star not detected, only lower limit can be given.
References: $^1$~this paper; $^2$ \citet{Egan}; $^3$ \citet{2000AetA...363..744G};
$^4$ \citet{1998MNRAS.301..640W}\label{Fluxes}. }
%\centering
\par
\begin{tabular}{lcccccl}
\hline
\hline
 Wavelength & Flux      & Error & Photometric aperture        &Instrument& SED  &Note       \\
\micron   &  [Jy]     &       &  Radius [~\arcsec{}~]    &                  & Fit? & Ref.\\
\hline
  1.6     & 1.1 $\times$ $10^{-4}$      & $\pm$12\% & 1.02$^a$   & ISAAC SWI & No  & $^1$\\
  2.2    & 1.5 $\times$ $10^{-2}$      & $^{+3.5}_{-2}$\% & 1.02$^a$   &ISAAC SWI & No&  $^1$  \\
\hline
  3.78    & 0.53          &$\simeq$8\%           & 4.6           & ISAAC LWI& No & $^1$ \\
  4.09  & 1.175         &$\simeq$11\%          & 4.6           & ISAAC LWI& No   &$^{1,\;b}$\\
  4.66     & 0.95        &$\simeq$8\%   & 4.6           & ISAAC LWI&No & $^{1,\;c}$\\
\hline
  11.9  & 10.52       &$\simeq$$10$\%  & 4.6           &TIMMI2& No & $^1$     \\
  12.9  & 10.7        &$\simeq$$10$\%  &  5.5          &TIMMI2& No & $^1$     \\
  20    & $>$29.5    & --    &      0.8        &TIMMI2& No & $^{1,\;d}$\\
\hline  
 8.28   & 30.74       & $\pm$5\%      &  PSF-Fit             & MSX A&  No &    $^2$ \\ 
 12     & 203       &$\pm$9\%       &  90             & IRAS& No&       $^3$   \\ 
 12.13  & 103.3       &$\pm$3\%       & PSF-Fit              & MSX C&  Yes&  $^2$    \\ 
 14.65  & 188.8       &$\pm$4\%       & PSF-Fit              & MSX D&  Yes &  $^2$   \\ 
 21.34  & 1301        &$\pm$6\%       & PSF-Fit              & MSX E&   Yes& $^2$    \\ 
 25     & 2577        &$\pm$4\%       &  90             & IRAS&   No &   $^3$  \\ 
 60     & 13611       &$\pm$8\%       &  90             & IRAS&   Yes & $^3$    \\ 
 100    & 14057       &$\pm$8\%       & 90              & IRAS&   Yes&  $^3$    \\ 
 148    & 9127        &--  & 90          & TIFR & Yes & $^3$ \\
 209    & 4753        &--    & 90        & TIFR& Yes & $^3$ \\
 1.2 mm & 17.0        &$\pm$20\%       & 60            & SEST& Yes & $^1$  \\
 3.5 cm &2.67 	& $\pm$10\%     &  5    & ATCA& No & $^{1,\;4}$     \\ 
 \hline
\end{tabular}
\end{table}