\begin{table}%t7
\footnotesize
\caption {\label{tab:crresults}Results of the gamma-ray emissivity analysis of the LMC for hypotheses \hone\ and \htwo.}
%\centerline
 {\begin{tabular}{lrr}
\hline\hline
\noalign{\smallskip}
Parameter & \multicolumn{1}{c}{\hone} & \multicolumn{1}{c}{\htwo} \\
\hline
$\Phi_{\gamma}$ & $25.0\pm1.7\pm4.1$ & $15.2\pm1.9\pm3.4$ \\
$q_{\gamma}$ & $6.9 \pm 2.4 \pm 2.6$ & $4.2 \pm 1.5 \pm 1.7$ \\
$r_{\rm c}$ & $ 0.31 \pm  0.01 \pm  0.02~^{+0.13}_{-0.07}$ & $0.21 \pm 0.01 \pm  0.02~^{+0.09}_{-0.05}$ \\
\hline
\end{tabular}}
\tablefoot {Given are the integrated $>100$~MeV photon flux $\Phi_{\gamma}$ in units of $10^{-8}$ \funit,
the average $>$100~MeV gamma-ray emissivity $q_{\gamma}$ in units of $10^{-27}$~\qunit,
and the cosmic-ray enhancement factor $r_{\rm c}$.
Quoted errors are statistic and systematic.
For $r_{\rm c}$ we quote in addition the (asymmetric) systematic error related to the
uncertainty in the total LMC gas mass.}
\end{table}