\begin{table}%t6
%\footnotesize
\caption {\label{tab:spectralfits}Maximum likelihood spectral fit results.}
%\centerline
 {
\begin{tabular}{lrrr}
\hline\hline
Parameter & \multicolumn{1}{c}{Total} & \multicolumn{1}{c}{Disk} & \multicolumn{1}{c}{30~Doradus} \\
\hline
Photon flux ($>$100 MeV) & $26.3\pm2.0\pm4.2$ & $18.4\pm2.3\pm3.0$ & $6.9\pm1.7\pm0.7$ \\
Energy flux ($>$100 MeV) & $16.0\pm0.6\pm1.8$ & $11.1\pm0.7\pm1.5$ & $4.6\pm0.5\pm0.5$ \\
Photon flux ($>$200 MeV) & $12.2\pm0.4\pm0.7$ & $8.3\pm0.6\pm0.7$ & $3.3\pm0.4\pm0.3$ \\
Energy flux ($>$200 MeV) & $12.9\pm0.4\pm1.8$ & $8.9\pm0.5\pm1.6$ &  $3.8\pm0.3\pm0.5$ \\
$\Gamma$ & $2.04\pm0.09\pm0.07$ & $2.10\pm0.13\pm0.10$ & $1.96\pm0.25\pm0.02$ \\
\ecut\ (GeV) & $\rm 7.1^{+3.5+6.6}_{-2.1-2.4}$ & $10.3^{+12.4+\infty}_{-4.4-10.3}$ & $\rm 6.9^{+10.5+1.3}_{-3.5-1.0}$ \\
TS with respect to power law & 11.3 & 3.0 & 3.6 \\
Significance of cut off ($\sigma$) & 3.4 & 1.7 & 1.9 \\
\hline
\end{tabular}}
\par
\tablefoot{Photon fluxes are given in units of $10^{-8}$ \funit,
energy fluxes are given in units of $10^{-11}$ \eunit.
Errors are statistical and systematic.}
\end{table}