\begin{table}%t2
\caption{\label{specfit-TZTZPM}Best fit parameters of a \textit{mekal} plus an absorbed power-law model for the \chandra\ data and an absorbed power-law model for the \xmm\ spectra.}
\newcommand{\T}{\rule{0pt}{2.6ex}}
\newcommand{\B}{\rule[-1.2ex]{0pt}{0pt}}
\par
%\centering
\par
  {
\begin{tabular}{l c c c c c c c c}
\hline
\hline \noalign{\smallskip}
Obs. ID \T \B & Nh\tablefootmark{a} &$\Gamma$ & Pl norm. & {\it kT}\tablefootmark{a} & $EM^{ab}$ & Flux\tablefootmark{c} & Corr. flux\tablefootmark{c} & Pl\tablefootmark{d}\\
 & $10^{20}$~cm$^{-2}$ & & $10^{-4}$~Photons~keV$^{-1}$~cm$^{-2}$~s$^{-1}$ &  keV & 10$^{62}$~cm$^{-3}$ & $10^{-13}$~erg~s$^{-1}$ & $10^{-13}$~erg~s$^{-1}$ & \%\ \\ 
\hline
 4741\T & $<$6.78 & 2.13~[2.00--2.28] & 4.28~[3.92--4.71] & 0.62~[0.58--0.66]  & 2.64~[2.27--2.99] & 18.1~[17.1--18.8] & 18.5~[18.2--20.1] & 94\\
 7077\T & & 2.26~[2.16--2.39] & 1.82~[1.68--1.99] &  &  & 7.8~[7.5--7.9] & 8.21~[8.0--9.0] & 83\\
 7078\T & & 2.34~[2.22--2.47] & 4.21~[3.90--4.61] &  &  & 16.0~[14.9--16.2] & 16.5~[16.1--18.5] & 93\\
 7079\T & & 2.38~[2.28--2.50] & 3.76~[3.54--4.07] &  &  & 14.1~[13.3--14.3] & 15.05~[14.7--16.4] & 90\\
 7080\T \B & & 2.02~[1.84--2.20] & 1.10~[0.96--1.26] &  & & 5.9~[5.5--6.1] & 6.0~[5.7--6.8] & 80\\
 7081\T \B & & 2.12~[2.00--2.25] & 1.25~[1.14--1.29] &  & & 6.2~[5.9--6.4] & 6.4~[6.2--7.1] & 81\\
\hline
\multicolumn{9}{c}{Reduced $\chi^{2} = 0.93$ for 310 d.o.f.} \T \B \\
\hline
 0205010101 \T \B & 3.82~[3.05--4.59] & 2.05~[2.03--2.07]  & 8.07~[7.90--8.24] & & & 33.8~[32.8--33.2]& 34.5~[34.2--34.8] & 100 \\
\hline
\multicolumn{9}{c}{Reduced $\chi^{2} = 1.01$ for 487 d.o.f.} \T \B \\
\hline
\end{tabular}}
\tablefoot {\tablefoottext{a}{Parameter linked for the different \chandra\ observations;}
\tablefoottext{b}{the emission measure (EM) of the \textit{mekal} model, $EM=\int$$n_{\rm e}$$n_{\rm H}$d$V$;}
\tablefoottext{c}{fluxes in the 0.5$-$8~keV energy range;}
\tablefoottext{d}{the power-law component fraction to the total corrected flux.}}
\end{table}