\begin{table}%t6
\caption{\label{tab:ATLAS9abundances}Abundances from ATLAS9 models computed for [M/H]~=~0.0
and microturbulent velocity $\xi=0$~km~s$^{-1}$. At this step
the helium abundance was assumed solar. 
%Errors are given only for lines with measured 
%equivalent widths, and no errors are presented for lines with abundances from comparison of observed and computed profiles
%using synthetic spectrum method. For \ion{Mn}{i} we did not use equivalent
%widths because Mn is affected by hyperfine structure. The hyperfine components are
%considered in the synthetic spectrum,
} 
%\centering
\par
\small\begin{tabular}{rrrrrrrrrr}
\hline\hline
\noalign{\smallskip}
\multicolumn{1}{c}{Elem.} & 
\multicolumn{1}{c}{T183}& 
\multicolumn{1}{c}{T191} & 
\multicolumn{1}{c}{T193}&
\multicolumn{1}{c}{NGC~6397}&
\multicolumn{1}{c}{B652}&
\multicolumn{1}{c}{B2151}&
\multicolumn{1}{c}{B2206}&
\multicolumn{1}{c}{NGC~6752}&
\multicolumn{1}{c}{Sun}
  \\
\noalign{\smallskip}
  &(11~480, 3.75) &(11~770, 3.8) &(11~480, 3.80)& &(12~250, 3.95) &(11~400, 3.85) &(11~290, 3.80) & & \\
\hline
\noalign{\smallskip}
\ion{C}{ii} &$\le$$-$5.02      &$\le$$-$5.02 &$\le$$-$5.02 &$-$5.43&$\le$$-$4.52 &$\le$$-$4.52 &$\le$$-$4.52&$-$5.13 & $-$3.52 \\
\ion{N}{i} &$\le$$-$5.12      &$\le$$-$5.12 &$\le$$-$5.12 & $-$6.03&$\le$$-$5.12 &$\le$$-$5.82 &$\le$$-$5.82&$-$5.73& $-$4.12\\
\ion{O}{i}  &$\le$$-$5.21      &$-$4.80 &$\le$$-$5.51 &$-$5.12&$\le$$-$5.51 &$\le$$-$5.51 &$\le$$-$5.51 &$-$4.82& $-$3.21 \\
\ion{Na}{i} &$\le$$-$6.71      &$\le$$-$6.71 &$\le$$-$6.71 &$-$7.62&$-$5.90 &$\le$$-$6.71 &$-$6.45 &$-$7.32& $-$5.71 \\ 
\ion{Mg}{ii} & $-$6.11          &$-$6.38 & $-$6.00 &$-$6.37&$-$5.68 &$-$5.75 &$-$5.71 &$-$6.07& $-$4.46 \\
\ion{Al}{i} &$\le$$-$6.75      &$\le$$-$6.75 &$\le$$-$6.75 &$-$7.48&$\le$$-$7.15 &$\le$$-$7.25 &$\le$$-$7.00 & $-$7.18& $-$5.57 \\
\ion{Si}{ii} &$-$7.49           &$-$6.76 &$\le$$-$7.80 &$-$6.40&$\le$$-$7.60 &$\le$$-$7.70 &$\le$$-$8.00 & $-$6.10&$-$4.49\\
\ion{P}{ii} &$-$5.40           &$\le$$-$6.59 &$-$5.43~$\pm$~0.10 &$-$8.50&$-$4.89~$\pm$~0.25 &$-$5.53 &$-$5.60~$\pm$~0.10 &$-$8.20& $-$6.59\\
\ion{S}{ii}  &$\le$$-$6.21      &$\le$$-$6.41 &$\le$$-$6.21 &$-$6.62&$\le$$-$6.21 &$\le$$-$6.21 &$\le$$-$6.21 &$-$6.32& $-$4.71\\
\ion{Ca}{ii} &$-$5.88           &$-$5.53 &$-$6.22 &$-$7.59&$-$5.85 &$-$6.34 &$-$6.28 &$-$7.29 & $-$5.68 \\
\ion{Sc}{ii} &$\le$$-$9.87      &$\le$$-$9.87 &$\le$$-$10.37 &$-$10.78 &$\le$$-$9.87 &$\le$$-$10.37 &$\le$$-$10.37 &$-$10.48& $-$8.87 \\
\ion{Ti}{ii} & $-$6.34~$\pm$~0.09 &$-$5.31~$\pm$~0.11 & $-$6.69~$\pm$~0.09 &$-$8.93&$-$7.00~$\pm$~0.11 &$-$6.87~$\pm$~0.07 &$-$6.88~$\pm$~0.07 &$-$8.63&$-$7.02\\
%\ion{V}{ii}  &$\le$$-$8.54      &$\le$$-$9.54  &$\le$$-$8.54 &$-$9.95&$\le$$-$9.04 &$\le$$-$9.54 &$\le$$-$9.54 &$-$9.65& $-$8.04 \\  
\ion{Cr}{ii} &$-$7.05~$\pm$~0.05 &$-$6.43~$\pm$~0.03 &$-$6.54~$\pm$~0.05 &$-$8.28&$-$6.81~$\pm$~0.04 &$-$6.88~$\pm$~0.03 &$-$6.80~$\pm$~0.05 &$-$7.98&$-$6.37\\
\ion{Mn}{ii} &$-$6.05           &$-$5.35 &$-$5.44 &$-$8.56&$-$5.75 &$-$6.50 &$-$6.30 &$-$8.26&$-$6.65\\
\ion{Fe}{i} & $-$4.17~$\pm$~0.09  & $-$4.68~$\pm$~0.06 & $-$4.27~$\pm$~0.09 &$-$6.45& $-$3.80~$\pm$~0.11 & $-$4.18~$\pm$~0.05 & $-$4.21~$\pm$~0.05 &$-$6.15&$-$4.54\\
\ion{Fe}{ii}&$-$4.17~$\pm$~0.11 &$-$4.68~$\pm$~0.09&$-$4.27~$\pm$~0.10&$-$6.45&$-$3.80~$\pm$~0.09&$-$4.18~$\pm$~0.11&$-$4.21~$\pm$~0.08&$-$6.15&$-$4.54\\
\ion{Co}{ii} &$\le$$-$7.92 & $-$6.12  &$\le$$-$7.12&$-$9.03&$-$&$\le$$-$7.92&$\le$$-$7.92&$-$8.73&$-$7.12\\
\ion{Ni}{ii}&$-$6.14& $-$6.00 &$-$6.25 &$-$7.70&$-$6.30 &$-$6.60 &$-$6.60 &$-$7.40& $-$5.79\\
\ion{Sr}{ii} & $\le$$-$10.57&$\le$$-$10.07 &$\le$$-$10.07 &$-$10.98&$\le$$-$10.07 &$\le$$-$10.57 &$\le$$-$10.57 &$-$10.68& $-$9.07\\
\ion{Y}{ii} & $-$8.20&$-$8.20 &$-$8.15~$\pm$~0.05 &$-$11.71&$-$7.43~$\pm$~0.12 &$-$8.50 &$-$8.34~$\pm$~0.08 &$-$11.41& $-$9.80\\
\ion{Zr}{ii}& $-$11.35 &$-$11.35 &$-$11.35 &$-$11.35&$-$11.05&$-$11.05&$-$9.01&$-$11.05&$-$9.44\\
\hline
\noalign{\smallskip}
\end{tabular}
\end{table}