\begin{table}%t3
\caption{Abundances ($\log(N_{\rm X}/N_{\rm tot})$) of the program stars. }
\label{abundance_table}
\par
\small%\centerline
 {
\begin{tabular}{rrrrrrrrrr}
\hline
\hline
\multicolumn{2}{c}{ } & \multicolumn{7}{c}{$\delta$~Scuti stars} & Solar \\
At.N.&Element   & HD~127929    & HD~138918    & HD~143466    & HD~124675    & HD~124953    & HD~125161    & HD~127762  & Abundances \\
\hline
6 & C	        &$-3.40(-;1)  $&$-3.34(09;2) $&$-3.71(-;1)  $&	            &$-3.78(06;2) $&$-3.62(09;2) $&$-3.44(-;1)  $&$-3.65 $\\  
8 & O	        &$-3.41(-;1)  $&$-3.49(-;1)  $&	             &	            &	           & 	          &	         &$-3.38 $\\  
11& Na          &$-5.76(06;2) $&$-5.57(10;2) $&	             &	            &$-5.65(01;2) $& 	          &	         &$-5.87 $\\  
12& Mg          &$-4.29(04;4) $&$-4.08(06;4) $&$-4.38(-;1)  $&$-4.77(11;3) $&$-4.51(10;5) $&$-4.39(09;2) $&$-4.29(01;2) $&$-4.51 $\\  
14& Si          &$-4.59(-;1)  $&$-4.64(-;1)  $&$-4.60(-;1)  $&$-4.50(-;1)  $&$-4.54(-;1)  $&$-4.36(-;1)  $&$-4.61(-;1)  $&$-4.53 $\\  
16& S	        &$-4.75(03;2) $&$-4.58(06;2) $&$-4.68(08;2) $&$-4.51(-;1)  $&$-4.63(07;5) $&$-4.28(05;2) $&$-4.37(04;2) $&$-4.90 $\\  
20& Ca          &$-5.54(11;7) $&$-5.35(14;9) $&$-5.52(01;2) $&$-5.72(-;1)  $&$-5.85(09;5) $&$-5.73(07;6) $&$-5.66(10;5) $&$-5.73 $\\  
21& Sc          &$-8.91(11;3) $&$-9.09(04;2) $&$-8.76(04;2) $&$-8.84(15;3) $&$-9.24(13;4) $&$-8.99(01;2) $&$-8.84(07;3) $&$-8.99 $\\  
22& Ti          &$-6.98(11;4) $&$-6.93(13;7) $&$-6.69(13;2) $&$-6.89(01;2) $&$-6.86(13;7) $&$-6.77(11;7) $&$-7.04(09;4) $&$-7.14 $\\  
24& Cr          &$-6.36(07;3) $&$-6.06(12;3) $&$-6.02(-;1)  $&$-6.84(04;3) $&$-6.26(23;4) $&$-6.49(19;5) $&$-6.48(09;3) $&$-6.40 $\\  
25& Mn          &$-6.51(-;1)  $&$-6.20(09;2) $&	             &	            &$-6.51(05;6) $& 	          &$-6.36(-;1)  $&$-6.65 $\\  
26& \ion{Fe}{i} &$-4.44(05;26)$&$-4.26(10;40)$&$-4.54(06;16)$&$-4.85(11;27)$&$-4.38(08;65)$&$-4.56(08;31)$&$-4.58(11;29)$&        \\
26& \ion{Fe}{ii}&$-4.39(05;5) $&$-4.24(14;3) $&$-4.56(-;1)  $&$-4.71(-;1)  $&$-4.35(15;3) $&$-4.55(07;5) $&$-4.55(12;5) $&        \\
26& Fe          &$-4.43(06;31)$&$-4.26(10;43)$&$-4.54(06;17)$&$-4.85(12;28)$&$-4.37(08;68)$&$-4.55(08;36)$&$-4.58(11;34)$&$-4.59 $\\  
28& Ni          &$-5.92(11;2) $&$-5.53(11;4) $&	             &$-6.24(-;1)  $&$-5.73(09;5) $&$-5.92(07;3) $&$-6.04(08;2) $&$-5.81 $\\  
39& Y	        &$-9.57(-;1)  $&$-9.49(11;2) $&	             &$-9.73(-;1)  $&$-9.36(-;1)  $&$-9.47(-;1)  $&$-9.22(-;1)  $&$-9.83 $\\  
56& Ba          &$-9.49(-;1)  $&$-9.37(-;1)  $&$-9.19(-;1)  $&$-9.66(-;1)  $&$-8.91(-;1)  $&$-9.27(-;1)  $&$-9.35(-;1)  $&$-9.87 $\\  
\hline
&   \Teff       & 7600	       & 7800         & 7380	     & 7500	    & 7600         & 7700	  & 7800	 & \\
&   \logg       & 3.70	       & 3.50         & 3.90	     & 4.00	    & 4.10         & 4.45	  & 3.75	 & \\
&   \vmic       & 2.7	       & 2.6          & 2.7	     & 2.7	    & 2.6          & 2.6	  & 2.6 	 & \\
&   \vsini      & 73	       & 88           & 136	     & 121	    & 82	   & 131	  & 121 	 & \\
&$\sigma_{\rm abn}$& 0.23      & 0.23         & 0.26	     & 0.25         & 0.23	   & 0.26	  & 0.25	 & \\
\hline
\end{tabular}}
\medskip
The estimated internal errors in units of 0.01 dex and the number of selected 
lines are given in parentheses. Abundances obtained from one line have 
no error~($-$). The uncertainties on the fundamental parameters, \Teff, \logg, 
and \vmic\  are 200~K, 0.22~dex and 0.7~\kms. The uncertainty on \vsini\  is 5\%.
The estimated uncertainty on the abundances~($\sigma_{\rm abn}$), including 
contributions from the high~\vsini\  and uncertainties on \Teff\  and \vmic, 
are given in the last row of the table.
\end{table}