\begin{table}%t1
%\renewcommand{\arraystretch}{1}
\caption{Primary
  parameters. Column~(1): cluster name; Col.~(2): optical redshift
  (e.g. Smith et~al. \cite{Smith2005}; Bardeau et~al. \cite{Bardeau2006}); Cols.~(3, 4): sky
  coordinates in epoch J2000 of the cluster center; Col.~(5): hydrogen
  column density (Dickey \& Lockman \cite{Dickey1990}); Col.~(6): truncation radius
  corresponding to a $S/N$ of 3 of the observational surface
  brightness profile; Cols.~(7--9): bolometric luminosity including
  the $<0.2r_{500}$ region, excluding the $<$$0.2r_{500}$ region, and
  corrected for the $<$$0.2r_{500}$ region, respectively.}
  \label{t:global}
  \small
%\centerline
{\begin{tabular}{lcccccccc}
\hline
\hline
Name & $z_{\rm opt}$ & \multicolumn{2}{c}{\mbox{X-ray} centroid} & $N_{\rm H}$ & $r_{\rm t}$ & $L_{\rm bol}^{\rm incc}$ & $L_{\rm bol}^{\rm excc}$ & $L_{\rm bol}^{\rm corr}$ \\
%\hline
    &               &
RA & Dec    & $10^{22}$~cm$^{-2}$ & arcmin &
$10^{45}$erg/s & $10^{45}$erg/s & $10^{45}$erg/s \\
\hline
Abell~68    &  0.255 &    00   ~    37   ~  06.159 &$   +09  $~   09   ~   28.72   &  0.0493  &   6.1   & $  1.17  \pm  0.10 $ & $  0.63  \pm  0.07 $ & $  0.89  \pm  0.10  $\\
Abell~209   &  0.209 &    01   ~    31   ~  52.607 &$   -13  $~   36   ~   35.50   &  0.0164  &   7.4   & $  1.25  \pm  0.10 $ & $  0.80  \pm  0.07 $ & $  1.04  \pm  0.10  $\\
Abell~267   &  0.230 &    01   ~    52   ~  42.021 &$   +01  $~   00   ~   41.17   &  0.0280  &   5.3   & $  0.75  \pm  0.07 $ & $  0.35  \pm  0.04 $ & $  0.51  \pm  0.07  $\\
Abell~383   &  0.187 &    02   ~    48   ~  03.340 &$   -03  $~   31   ~   43.55   &  0.0392  &   7.7   & $  0.76  \pm  0.05 $ & $  0.25  \pm  0.04 $ & $  0.34  \pm  0.05  $\\
Abell~773   &  0.217 &    09   ~    17   ~  52.935 &$   +51  $~   43   ~   19.41   &  0.0144  &   7.7   & $  2.06  \pm  0.15 $ & $  1.05  \pm  0.11 $ & $  1.50  \pm  0.15  $\\
Abell~963   &  0.206 &    10   ~    17   ~  03.178 &$   +39  $~   02   ~   56.53   &  0.0140  &   6.1   & $  1.16  \pm  0.09 $ & $  0.56  \pm  0.07 $ & $  0.75  \pm  0.09  $\\
Abell~1689  &  0.184 &    13   ~    11   ~  29.330 &$   -01  $~   20   ~   26.66   &  0.0182  &   8.0   & $  2.94  \pm  0.10 $ & $  0.96  \pm  0.06 $ & $  1.49  \pm  0.10  $\\
Abell~1763  &  0.228 &    13   ~    35   ~  18.115 &$   +41  $~   00   ~   03.89   &  0.0936  &   7.5   & $  1.75  \pm  0.15 $ & $  1.21  \pm  0.12 $ & $  1.50  \pm  0.15  $\\
Abell~1835  &  0.253 &    14   ~    01   ~  01.865 &$   +02  $~   52   ~   35.48   &  0.0232  &   7.0   & $  5.18  \pm  0.17 $ & $  1.56  \pm  0.10 $ & $  2.29  \pm  0.17  $\\
Abell~2218  &  0.176 &    16   ~    35   ~  53.775 &$   +66  $~   12   ~   32.43   &  0.0324  &   7.7   & $  1.15  \pm  0.08 $ & $  0.70  \pm  0.06 $ & $  0.94  \pm  0.08  $\\
Abell~2219  &  0.226 &   16   ~   40   ~ 19.900 &  $+46$ ~   42   ~  41.00   &  0.0178  & ---     & ---                  & ---                   & --- \\
Abell~2390  &  0.233 &    21   ~    53   ~  37.115 &$   +17  $~   41   ~   46.41   &  0.0680  &   7.7   & $  3.90  \pm  0.26 $ & $  1.86  \pm  0.17 $ & $  2.54  \pm  0.26  $\\
Abell~2667  &  0.230 &    23   ~    51   ~  39.218 &$   -26  $~   05   ~   03.49   &  0.0165  &   7.6   & $  2.10  \pm  0.12 $ & $  0.81  \pm  0.08 $ & $  1.11  \pm  0.12  $\\
\hline
  \end{tabular}}
\smallskip
The XMM-Newton observations of Abell~2219 are flared.
\end{table}