\begin{table}
%  %\centering
\par
%  \caption{Best-fit parameters to the continuum RGS spectrum of Mrk 279, consisting of a single power law plus a modified black body, for the $H$, $L$ and $R$ datasets. The continuum and black body luminosities are both in the 0.5-2~keV range.}
%  \label{cont}
%
%  \begin{tabular}{lcccc}
%    \hline
%    \hline
%    \noalign{\smallskip}
%    Dataset & $\Gamma$ & $L_{0.5-2~{\rm{~keV}}}$$^a$ & $T_{mbb}$ (keV)& $L_{mbb}$$^a$  \\
%    \noalign{\smallskip}
%    \hline
%    \noalign{\smallskip}
%    $H$ & 2.05$\pm$0.07 & 4.7$\pm$0.1 & 0.14$\pm$0.01 & 0.43$\pm$0.06 \\
%    \noalign{\smallskip}
%    \hline
%    \noalign{\smallskip}
%    $L$ & 1.91$\pm$0.08 & 3.9$\pm$0.1 & 0.14$\pm$0.01 & 0.43$\pm$0.05 \\ 
%    \noalign{\smallskip}
%    \hline
%    \noalign{\smallskip}
%    $R$ & 2.03$\pm$0.08 & 4.3$\pm$0.1 & 0.14$\pm$0.01 & 0.33$\pm$0.07 \\ 
%    \noalign{\smallskip}
%    \hline
%    \noalign{\smallskip}
%    \multicolumn{4}{l}{$^a$ In units of $10^{43}$~erg s$^{-1}$}\\
%  \end{tabular}
%\end{table}