\begin{table}%t5
     \caption{\label{SSC_results}Results of SSC fits to the SED of H~2356--309.}
       %\centerline
{\small
        \begin{tabular}{c c c c c}
           \hline\hline
           \noalign{\smallskip}
& XMM$_1$\tablefootmark{a}  & XMM$_2$$^a$ & RXTE$^{\dagger}$ & AH06\tablefootmark{c}\\
           \noalign{\smallskip}
           \hline
	$\delta$ & 18 & 18 & 18 & 18\\
	$B$ [G] & 0.16 & 0.16 & 0.16 & 0.16\\
	$R$ [cm] & $7.5 \times 10^{15}$ &  $7.5 \times 10^{15}$ &  $7.0 \times 10^{15}$ & $3.4 \times 10^{15}$\\
	$K$ [cm$^{-3}$] & $8.0 \times 10^{4}$ &  $8.0 \times 10^{4}$ & $2.0 \times 10^{4}$ & $1.2 \times 10^{4}$\\
	$\gamma_{\rm min}$ &  $1.0 \times 10^{3}$ & $1.0 \times 10^{3}$ & $1.0 \times 10^{3}$ & $1.0 \times 10^{3}$\\
	$\gamma_{\rm b}$ & $1.0 \times 10^{5}$ &  $1.0 \times 10^{5}$ & $2.5 \times 10^{5}$ & $2.5 \times 10^{5}$\\
	$\gamma_{\rm max}$ & $3.0 \times 10^{6}$ & $3.0 \times 10^{6}$ & $3.0 \times 10^{6}$ & $3.0 \times 10^{6}$\\
	$n_1$ & 2.3 & 2.3 & 2.0 & 2.0 \\
	$n_2$ & 3.6 & 3.5 & 3.4 & 4.0 \\
           \hline
      \end{tabular}}
    \tablefoot{\tablefoottext{a}{The XMM$_1$ and XMM$_2$ results refer to the fits to the data
from MJD 53~534 and 53~536, respectively.  Using the \mbox{XMM-Newton} optical
spectrum from MJD 53~536 instead of the average ROTSE-IIIc flux from 2004 for the RXTE campaign
yields the same SSC fit parameters as shown in XMM$_2$.}
\tablefoottext{b}{This is the result of the original SSC modeling of the RXTE campaign SED of H~2356--309 published in \cite{HESS_MWLI}.  The RXTE$^{\dagger}$ results use the same multi-wavelength data as AH06 along with an improved calibration of the VHE data.}}
  \end{table}