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\begin{document}

\setcounter{table}{3}
\begin{table}%{4}
%\centering
%\par
\caption{Abundances (scaled to the solar ratio) obtained from the EPIC analysis for each cluster. 
Values with errors larger than 3~times solar are not presented 
(indicated by $-$).\label{tbl:eack-abun}}
\begin{tabular}{rrrrr}
\hline \hline 
$R^{{a}}$ & Fe/H& O/Fe& Si/Fe & S/Fe\\
\hline 
\multicolumn{5}{c}{NGC~533} \\ 
\#0  & $0.39\pm {0.06}$  & $ 0.3\pm { 0.7}$  & $ 1.6\pm { 0.7}$  & $ 2.8\pm { 1.3}$ \\ 
\#1  & $0.26\pm {0.09}$  & $ 1.9\pm { 1.9}$  & $ 1.7\pm { 1.2}$  & $ 1.1\pm { 1.7}$ \\ 
\hline 
\multicolumn{5}{c}{A 262} \\ 
\#0  & $0.67\pm {0.05}$  & $ 0.6\pm { 0.3}$  & $ 1.4\pm { 0.2}$  & $ 1.0\pm { 0.3}$ \\ 
\#1  & $0.34\pm {0.04}$  & $ 1.8\pm { 0.9}$  & $ 1.2\pm { 0.4}$  & $ 0.7\pm { 0.5}$ \\ 
\hline 
\multicolumn{5}{c}{A 1837} \\ 
\#0  & $0.64\pm {0.14}$  & $ 0.5\pm { 1.6}$  & $ 2.8\pm { 1.6}$  & $ 1.0\pm { 1.4}$ \\ 
\#1  & $0.39\pm {0.07}$  & $ 0.9\pm { 1.1}$  & $ 0.9\pm { 0.7}$  & $ 0.4\pm { 0.8}$ \\ 
\#2  & $0.27\pm {0.13}$  & $ 1.7\pm { 3.0}$  & $ 1.0\pm { 1.6}$  & $ 3.7\pm { 2.9}$ \\ 
\hline 
\multicolumn{5}{c}{S\'ersic 159$-$3} \\ 
\#0  & $0.39\pm {0.03}$  & $ 0.6\pm { 0.4}$  & $ 1.3\pm { 0.2}$  & $ 0.8\pm { 0.3}$ \\ 
\#1  & $0.23\pm {0.03}$  & $ 0.8\pm { 0.8}$  & $ 1.4\pm { 0.6}$  & $ 0.5\pm { 0.5}$ \\ 
\#2  & $0.09\pm {0.05}$ & --  & $ 1.5\pm { 1.7}$  & $ 1.5\pm { 2.7}$ \\ 
\hline 
\multicolumn{5}{c}{MKW 9} \\ 
\#0  & $0.63\pm {0.15}$  & $ 0.1\pm { 0.5}$  & $ 1.9\pm { 0.7}$  & $ 1.4\pm { 0.8}$ \\ 
\#1  & $0.97\pm {0.45}$ & --  & $ 0.2\pm { 0.8}$  & $ 0.0\pm { 0.7}$ \\ 
\hline 
\multicolumn{5}{c}{2A 0335+096} \\ 
\#0  & $0.60\pm {0.04}$  & $ 1.6\pm { 0.7}$  & $ 1.0\pm { 0.2}$  & $ 0.8\pm { 0.3}$ \\ 
\#1  & $0.42\pm {0.07}$  & $ 1.8\pm { 1.7}$  & $ 1.2\pm { 0.6}$  & $ 0.0\pm { 0.4}$ \\ 
\#2  & $0.31\pm {0.17}$ & --  & $ 0.3\pm { 1.1}$  & $ 1.5\pm { 1.9}$ \\ 
\hline 
\multicolumn{5}{c}{MKW 3s} \\ 
\#0  & $0.68\pm {0.06}$  & $ 0.5\pm { 0.4}$  & $ 1.4\pm { 0.3}$  & $ 0.9\pm { 0.4}$ \\ 
\#1  & $0.31\pm {0.03}$  & $ 1.3\pm { 0.9}$  & $ 1.5\pm { 0.6}$  & $ 0.5\pm { 0.5}$ \\ 
\#2  & $0.09\pm {0.06}$  & $ 0.0\pm { 1.9}$ & -- & -- \\ 
\hline 
\multicolumn{5}{c}{A 2052} \\ 
\#0  & $0.58\pm {0.04}$  & $ 0.7\pm { 0.4}$  & $ 1.3\pm { 0.3}$  & $ 0.8\pm { 0.3}$ \\ 
\#1  & $0.41\pm {0.04}$  & $ 0.6\pm { 0.5}$  & $ 1.4\pm { 0.5}$  & $ 0.6\pm { 0.5}$ \\ 
\#2  & $0.13\pm {0.06}$ & --  & $ 0.3\pm { 1.1}$  & $ 3.3\pm { 2.6}$ \\ 
\hline 
\multicolumn{5}{c}{A 4059} \\ 
\#0  & $0.72\pm {0.12}$  & $ 0.5\pm { 0.6}$  & $ 1.3\pm { 0.6}$  & $ 1.7\pm { 0.8}$ \\ 
\#1  & $0.44\pm {0.08}$  & $ 0.7\pm { 0.7}$  & $ 1.4\pm { 0.9}$  & $ 0.7\pm { 0.8}$ \\ 
\#2  & $0.41\pm {0.23}$  & $ 1.2\pm { 2.5}$  & $ 3.2\pm { 2.2}$  & $ 1.7\pm { 2.5}$ \\ 
\hline 
\multicolumn{5}{c}{Hyd A} \\ 
\#0  & $0.42\pm {0.05}$  & $ 0.8\pm { 0.6}$  & $ 1.1\pm { 0.5}$  & $ 0.4\pm { 0.5}$ \\ 
\#1  & $0.30\pm {0.05}$  & $ 0.9\pm { 0.8}$  & $ 1.9\pm { 0.9}$  & $ 0.7\pm { 0.8}$ \\ 
\#2  & $0.20\pm {0.11}$ & --  & $ 0.5\pm { 1.7}$  & $ 0.0\pm { 1.2}$ \\ 
\hline 
\end{tabular}
\begin{list}{}{}
\item[$^{{a}}$] Integration region (\#0, \#1, \#2 for radii
between 0--50, 50--200,
 and 200--500 in $h^{-1}$~kpc). 
\end{list}
\end{table}

%\clearpage
\setcounter{table}{3}
\begin{table}%{4}
%\centering
\par
\caption{Abundances obtained from the EPIC analysis 
for each cluster (continued).}
\begin{tabular}{rrrrr}
\hline \hline 
$R$	& Fe/H	& O/Fe & Si/Fe & S/Fe\\
\hline 
\multicolumn{5}{c}{A 496} \\ 
\#0  & $0.60\pm {0.05}$  & $ 0.4\pm { 0.3}$  & $ 1.6\pm { 0.3}$  & $ 1.1\pm { 0.4}$ \\ 
\#1  & $0.37\pm {0.07}$  & $ 1.5\pm { 1.2}$  & $ 1.5\pm { 0.8}$  & $ 0.7\pm { 0.8}$ \\ 
\#2  & $0.41\pm {0.26}$ & --  & $ 1.7\pm { 2.3}$  & $ 1.8\pm { 2.7}$ \\ 
\hline 
\multicolumn{5}{c}{A 3112} \\ 
\#0  & $0.70\pm {0.05}$  & $ 0.9\pm { 0.6}$  & $ 1.4\pm { 0.4}$  & $ 0.4\pm { 0.3}$ \\ 
\#1  & $0.36\pm {0.05}$  & $ 0.2\pm { 0.7}$  & $ 1.0\pm { 0.8}$  & $ 0.6\pm { 0.7}$ \\ 
\#2  & $0.22\pm {0.13}$  & $ 0.0\pm { 1.6}$  & $ 1.3\pm { 2.3}$  & $ 2.3\pm { 2.7}$ \\ 
\hline 
\multicolumn{5}{c}{A 1795} \\ 
\#0  & $0.51\pm {0.04}$  & $ 0.7\pm { 0.4}$  & $ 1.4\pm { 0.4}$  & $ 0.6\pm { 0.4}$ \\ 
\#1  & $0.32\pm {0.04}$  & $ 0.5\pm { 0.7}$  & $ 1.9\pm { 1.1}$  & $ 0.0\pm { 0.5}$ \\ 
\#2  & $0.26\pm {0.07}$  & $ 1.4\pm { 1.9}$  & $ 3.2\pm { 2.1}$  & $ 0.6\pm { 1.2}$ \\ 
\hline 
\multicolumn{5}{c}{A 399} \\ 
\#0  & $0.63\pm {0.35}$  & $ 0.0\pm { 2.2}$  & $ 0.0\pm { 1.2}$  & $ 0.0\pm { 1.4}$ \\ 
\#1  & $0.31\pm {0.12}$ & --  & $ 0.9\pm { 2.2}$ & -- \\ 
\#2  & $0.28\pm {0.13}$ & -- & -- & -- \\ 
\hline 
\multicolumn{5}{c}{A 3266} \\ 
\#0  & $0.46\pm {0.34}$ & -- & -- & -- \\ 
\#1  & $0.27\pm {0.13}$ & -- & -- & -- \\ 
\#2  & $0.22\pm {0.08}$ & -- & -- & -- \\ 
\hline 
\multicolumn{5}{c}{Perseus} \\ 
\#0  & $0.57\pm {0.03}$  & $ 1.4\pm { 0.3}$  & $ 1.2\pm { 0.2}$  & $ 0.4\pm { 0.4}$ \\ 
\#1  & $0.41\pm {0.04}$  & $ 2.3\pm { 0.9}$  & $ 1.2\pm { 0.4}$  & $ 0.2\pm { 0.3}$ \\ 
\hline 
\multicolumn{5}{c}{Coma} \\ 
\#0  & $0.53\pm {0.54}$ & -- & -- & -- \\ 
\#1  & $0.26\pm {0.09}$ & --  & $ 3.8\pm { 2.8}$  & $ 0.7\pm { 2.0}$ \\ 
\#2  & $0.25\pm {0.10}$  & $ 2.4\pm { 2.8}$  & $ 1.4\pm { 2.1}$  & $ 0.0\pm { 0.9}$ \\ 
\hline 
\multicolumn{5}{c}{A 754} \\ 
\#0  & $0.32\pm {0.34}$  & $ 0.0\pm { 2.5}$ & -- & -- \\ 
\#1  & $0.33\pm {0.11}$  & $ 1.1\pm { 2.2}$  & $ 0.4\pm { 1.4}$  & $ 0.6\pm { 1.6}$ \\ 
\#2  & $0.21\pm {0.09}$ & -- & -- & -- \\ 
\hline 
\multicolumn{5}{c}{A 1835} \\ 
\#0  & $0.42\pm {0.06}$  & $ 2.0\pm { 1.4}$  & $ 1.1\pm { 0.9}$  & $ 0.6\pm { 1.0}$ \\ 
\#1  & $0.38\pm {0.09}$  & $ 0.0\pm { 1.0}$  & $ 0.0\pm { 0.6}$  & $ 0.0\pm { 1.1}$ \\ 
\#2  & $0.29\pm {0.11}$ & -- & --  & $ 1.7\pm { 2.8}$ \\ 
\hline
\end{tabular}
\end{table}

\end{document}
