\begin{table}%t1
 \caption{Photon energy spectra and luminosity (0.2 to 10~TeV) of the VHE $\gamma$-ray emission of LS~5039 for different orbital phase intervals.
   The broad phase intervals \textbf{INFC} and \textbf{SUPC} encompass the inferior and superior conjunction epochs.
   The orbital phase $\phi$ is calculated from the ephemeris of Casares \etal (\cite{Casares:1}). The best-fit 
   function is indicated for each phase interval. The errors quoted are statistical with systematic errors in the~10 to 15\% range.
 \label{tab:spec}}
%\begin{center}
 { \begin{tabular}{c|cccc} \hline \hline
%&&&\\[-2mm]
   Orbital phase interval & $N$               & $\Gamma$ & $E_{\rm o}$ & Luminosity$^\dagger$ \\
   &  $\times 10^{-12}$ [ph~cm$^{-2}$~s$^{-1}$~TeV$^{-1}$] & & [TeV] & [erg~s$^{-1}$]\\ \hline %\vspace*{2mm}
   \multicolumn{5}{c}{Fit function:  \fbox{${\rm d}N/{\rm d}E = N E^{-\Gamma} \exp~(-E/E_{\rm o})$}} \\ \hline%&&&\\[-2mm]
   \textbf{INFC} ($0.45<\phi\leq0.9$) & $2.28 \pm0.10$ & $1.85\pm0.06$ & $8.7\pm2.0$ & $1.1\times 10^{34}$\\
   \textbf{SUPC} ($\phi \leq 0.45$) and $\phi>0.9$  & $0.91 \pm0.07$  & $2.53\pm0.07$ & -- & $4.2\times 10^{33}$\\
   All Phases (time averaged)  & $1.85 \pm0.06$  & $2.06\pm0.05$ & $13.0\pm4.1$ & $7.8\times 10^{33}$\\ \hline
   \noalign{\smallskip}
   \multicolumn{5}{c}{Power-Law fit for energies $E\leq5$~TeV (narrow phase intervals)}\\ \hline
  % &&&\\[-2mm]
   0.0--0.1 & 0.84 $\pm$ 0.17 & 2.62 $\pm$ 0.23 & & \\
   0.1--0.2 & 0.46 $\pm$ 0.21 & 3.08 $\pm$ 0.47 & & \\
   0.2--0.3 & 0.81 $\pm$ 0.13 & 2.46 $\pm$ 0.20 & & \\
   0.3--0.4 & 0.78 $\pm$ 0.18 & 2.77 $\pm$ 0.60 & & \\
   0.4--0.5 & 1.88 $\pm$ 0.27 & 2.32 $\pm$ 0.17 & & \\
   0.5--0.6 & 2.64 $\pm$ 0.20 & 2.04 $\pm$ 0.10 & & \\
   0.6--0.7 & 2.20 $\pm$ 0.23 & 1.88 $\pm$ 0.13 & & \\
   0.7--0.8 & 2.44 $\pm$ 0.20 & 1.90 $\pm$ 0.10 & & \\
   0.8--0.9 & 2.96 $\pm$ 0.17 & 1.94 $\pm$ 0.08 & & \\
   0.9--1.0 & 1.21 $\pm$ 0.25 & 1.84 $\pm$ 0.25 & & \\ \hline
 \end{tabular}}
%\end{center}
\par
\hspace{2.3cm}{$\dagger$ At 2.5~kpc distance.}
%\vspace{-3mm}
\end{table}