\begin{table}%t3
\caption{Equivalent width (EW) measurements of the emission line
	objects. \emph{Upper table}: Cols.~2--7 give the EW for the
	spectral lines in the \brg\ setting. The EWs are measured in \AA
	ngstr\"{o}m and emission is given as positive. In Col. 8 the
	{\it FWHM} of \brg\ is given in \kms. Columns 9 and 10 show whether
	the CO and Pfund-lines are present in the spectra or
	not. ("--'' means not present, "n'' means not
	observed). \emph{Middle table}: the EW measurements of the
	Pf-lines. The "b'' means that the line could not be measured
	because of blending with the CO lines.  The Pf-lines of
	\object{16571nr1281} are double peaked with an average peak
	separation of $189 \pm 33$~\kms. \emph{Lower table}: the EW
	measurements of the CO first-overtone bandheads. The "b''
	means that the lines are blended with cold CO absorption lines
	or Pfund lines.\label{tab:ew}} {
%\centering
\par
%\begin{tabular}{llllllllllll}\hline\hline
 \begin{tabular}{p{1.7cm}p{1.3cm}p{1.3cm}p{1.5cm}p{1.3cm}p{1.3cm}p{1.7cm}p{1.3cm}p{1.3cm}p{1.3cm}p{1.3cm}p{1.5cm}}\hline\hline
\multicolumn{1}{c}{Object}&\multicolumn{1}{c}{\ion{Fe}{ii} (2.09)}& \multicolumn{1}{c}{\hei\ (2.1128)}& \multicolumn{1}{c}{\hei\ (2.1137)}& \multicolumn{1}{c}{\ion{Mg}{ii} (2.138)} & \multicolumn{1}{c}{\ion{Mg}{ii} (2.144)}&\multicolumn{1}{c}{ \brg\ (2.166)}   &\multicolumn{1}{c}{{\it FWHM}(\brg)}  &\multicolumn{1}{c}{CO}    & \multicolumn{1}{c}{Pf} & &  \\ \hline
\noalign{\smallskip}
\object{06058nr227}  &--	    	    &--	    	   &-- 	    	    &--	     	  &--   	    &\raggedleft1.53 $\pm$  0.10 & \raggedleft 182 $\pm$ 6   & n    &  n   & & \\
\object{06058nr221}  &--	    	    &--	    	   &-- 	    	    &--	     	  &--   	    &\raggedleft36.41 $\pm$ 1.31 &\raggedleft 202 $\pm$ 1   & n    &  n  & & \\
\object{06061nr676}  &--	    	    &--	    	   &-- 	    	    &--	     	  &--   	    &\raggedleft33.22 $\pm$  0.34&\raggedleft 166 $\pm$ 11  & n    &  n   & & \\
\object{06084nr118}  &0.60 $\pm$ 0.04          &--	    	   &-- 	    	    &--	    	  &--   	    &\raggedleft111.1 $\pm$  0.12&\raggedleft 156 $\pm$ 1   & n    &  n  & &  \\
\object{06084nr114}  &--	    	    &--	    	   &-- 	    	    &--	     	  &--   	    &\raggedleft1.51 $\pm$  0.11 &\raggedleft 212 $\pm$ 8   & n    &  n   & & \\
\object{06412nr121}  & --	            &0.13 $\pm$ 0.03 & 0.07 $\pm$ 0.03  &0.78 $\pm$ 0.18&0.76 $\pm$ 0.17    &\raggedleft12.2 $\pm$  0.08 & \raggedleft147 $\pm$ 1   & --   &  +   & &\\
\object{07299nr598}  &0.24 $\pm$ 0.04         &--	    	   &-- 	    	    &-- 	  &--   	    &\raggedleft19.6 $\pm$  0.13 &\raggedleft 217 $\pm$ 1   & --   &  -- & & \\
\object{07299nr618}  &0.48 $\pm$ 0.04         &--	    	   &-- 	    	    &-- 	  &--   	    &\raggedleft4.12 $\pm$  0.06 &\raggedleft 138 $\pm$ 2   & +    &  -- & & \\
\object{07299nr43}   &0.53 $\pm$ 0.05         &--	    	   &-- 	    	    &0.28 $\pm$ 0.11&0.25\raggedleft $\pm$ 0.16    &\raggedleft4.87 $\pm$  0.08 &\raggedleft 146 $\pm$ 1   & --   &  -- & & \\
\object{07299nr314}  &1.43 $\pm$ 0.06         &--	    	   &-- 	    	    &-- 	  &--  	    	    &\raggedleft14.9 $\pm$  0.11 &\raggedleft 115 $\pm$ 2   & --   &  -- & &  \\
\object{08576nr292}  &--	    	    &--	    	   &-- 	    	    &-- 	  &--  	    	    &\raggedleft15.1 $\pm$  0.16 & \raggedleft220 $\pm$ 2   & +    &  -- & & \\
\object{08576nr408}  & --	            &--	    	   &-- 	    	    &--     	  &--  	    	    &\raggedleft3.88 $\pm$  0.09 &\raggedleft 181 $\pm$ 2   & --   &  -- & & \\
\object{11097nr1218} &--	    	    &--	    	   &-- 	    	    &-- 	  &--  	    	    &\raggedleft4.83 $\pm$  0.08 &\raggedleft 191 $\pm$ 3   & +    &  -- & & \\
\object{11097nr693}  &--	    	    &--	    	   &-- 	    	    &-- 	  &--  	    	    &\raggedleft6.73 $\pm$  0.07 &\raggedleft 121 $\pm$ 1   & --   &  -- & & \\
\object{15411nr1955} &0.22 $\pm$ 0.04         &--	    	   &-- 	    	    &0.47 $\pm$ 0.10&0.34 $\pm$ 0.10    &\raggedleft6.99 $\pm$  0.06 &\raggedleft 106 $\pm$ 1   & --   &  +  & & \\
\object{16164nr3636} &--	    	    &2.15 $\pm$ 0.22 &-- 	    	    &2.17 $\pm$ 0.15&1.25 $\pm$ 0.24    &\raggedleft16.66 $\pm$  0.10&\raggedleft 132 $\pm$ 1   & +    &  +  & & \\
\object{16571nr1281} &--	    	    &--	    	   &-- 	    	    &--	     	  &--  	    	    &\raggedleft10.65 $\pm$  0.13&\raggedleft 204 $\pm$ 1   & --   &  +  & & \\
\object{17136nr649}  &--	    	    &--	    	   &-- 	    	    &--	     	  &--  	            &\raggedleft6.06 $\pm$  0.10 &\raggedleft 182 $\pm$ 2   & --   &  -- & & \\
\object{17258nr593}  &1.61 $\pm$ 0.04         &--	    	   &-- 	    	    &0.33 $\pm$ 0.10&0.67 $\pm$ 0.20    &\raggedleft7.98 $\pm$  0.06 &\raggedleft 118 $\pm$ 2   & --   & --  & & \\
\object{18006nr766}  &--	    	    &0.13 $\pm$ 0.03 &0.06 $\pm$ 0.04   &--	     	  &--  	            &\raggedleft10.65 $\pm$  0.08&  \raggedleft 99 $\pm$ 1    & +    &  +  & & \\
\object{18507nr248}  &--	    	    &--	    	   &-- 	    	    &--	     	  &--  	   	    &\raggedleft6.41 $\pm$  0.07 &\raggedleft 154 $\pm$ 1   & --   &  -- & & \\ \hline\hline
\multicolumn{1}{c}{Object}& \multicolumn{1}{c}{Pf23}& \multicolumn{1}{c}{Pf24}& \multicolumn{1}{c}{Pf25}& \multicolumn{1}{c}{Pf26}& \multicolumn{1}{c}{Pf27}& \multicolumn{1}{c}{Pf28}& \multicolumn{1}{c}{Pf29}& \multicolumn{1}{c}{Pf30}& \multicolumn{1}{c}{Pf31}& \multicolumn{1}{c}{Pf32}& \multicolumn{1}{c}{Pf33} \\ \hline
\noalign{\smallskip}
\object{06412nr121}  & 4.45 $\pm$ 0.23 & 3.27 $\pm$ 0.28& 3.76  $\pm$ 0.26 &2.61 $\pm$ 0.27&2.58 $\pm$ 0.26    & 2.00 $\pm$ 0.25 &1.04 $\pm$ 0.23&0.94 $\pm$ 0.21 & 0.50 $\pm$ 0.11 & 0.66 $\pm$ 0.18  & 0.67 $\pm$  0.25 \\
\object{154111995}   & 0.53 $\pm$ 0.01 & 0.41 $\pm$ 0.01& 0.43  $\pm$ 0.01 &--           &--               & --            & --          & --           & --            &  --            & --             \\
\object{16164nr336}  & 3.15 $\pm$ 0.17 & b            & 3.46  $\pm$ 0.19 &3.20 $\pm$ 0.20& 3.35 $\pm$ 0.21   & b             & 1.85 $\pm$ 0.19& 2.00 $\pm$ 0.18& --           & --             & --             \\
\object{16571nr1281} & 2.81 $\pm$ 0.10 & 2.29 $\pm$ 0.10& 2.01 $\pm$ 0.10  &1.33 $\pm$ 0.10&1.34 $\pm$ 0.10    & 1.02 $\pm$ 0.10 & 0.88 $\pm$ 0.09& 0.53 $\pm$ 0.08& 0.47 $\pm$ 0.13& 0.52 $\pm$ 0.15  & 0.55 $\pm$ 0.23 \\
\object{18006nr766}  & 1.06 $\pm$ 0.06 & --           & --             &--           &--               & --            & --          & --           & --            &  --            & --             \\ \hline \hline
\multicolumn{1}{c}{Object}      & \multicolumn{1}{c}{CO(2--0)}       & \multicolumn{1}{c}{CO(3--1)}      & \multicolumn{1}{c}{CO(4--2)}        & \multicolumn{1}{c}{CO (5--3)}    &                 &               &             &              &               &                &                \\ \hline
\noalign{\smallskip}
\object{07299nr618}  &\raggedleft 4.0          &\raggedleft b            & \raggedleft   b           &\raggedleft 1.0        &                 &               &             &              &               &                &                \\ 
\object{08576nr292}  &\raggedleft 67.1        &\raggedleft 76.5        &\raggedleft    64.5       &\raggedleft  32.3       &                 &               &             &              &               &                &                \\ 
\object{11097nr1218} &\raggedleft 25.0         &\raggedleft  28.7       & \raggedleft     28.7      &\raggedleft  19.1      &                 &               &             &              &               &                &                \\ 
\object{16164nr3636} &\raggedleft 12.4          &\raggedleft b            &\raggedleft     b          &\raggedleft  b          &                 &               &             &              &               &                &                \\ 
\object{18006nr766}  &\raggedleft 17.2         &\raggedleft 16.2        &\raggedleft 12.2          & \raggedleft b          &                 &               &             &              &             
  &                &                \\ \hline
\end{tabular}}
\end{table}