\begin{table}%t2
%\centering
\par
\caption{Derived stellar atmosphere parameters and elemental abundances for the sample.  The entire table is available only electronically.  This portion of the table is given as a guide to its form.  For each star we report the average signal-to-noise ratio per pixel for the whole observed spectrum, the stellar parameters with their respective relative and absolute rms error estimates,  $\sigma^{\rm rel}$ and $\sigma^{\rm abs}$, then for each element X the abundance $\log \epsilon_{\rm X}$ and its relative and absolute rms error estimates $\sigma_{\log\epsilon_{\rm X}}$, [X/Fe] and its relative and absolute rms error estimates $\sigma_{\rm [X/Fe]}$.  $N$ gives the number of features of the element used in each star, noting that this varies from star to star as certain features may be automatically rejected if the star has a strong G~band, if the feature is near a Balmer line in warmer stars (see Sect.~\ref{sect:lines}), or if they are determined to be affected by a cosmic ray hit or bad pixel. N3 then gives the number of those features classified as 3$\sigma$ detections.  In the case of 
CH~bands we simply classify detections and non-detections with~1 and 0~respectively.  In the case of a non-detection, this is signified by an abundance of $-9.99$ and error of $0.00$.
\label{tab:abunds}}
\scriptsize
%\tiny
\begin{tabular}{ccccccccccccccccrccccc}
\hline\hline
Star        & $S/N_{\rm av}$ & $T_{\rm eff}$ & $\sigma_{T_{\rm eff}}$  & $\log g$ & $\sigma_{\log g}^{\rm rel}$ & $\sigma_{\log g}^{\rm abs}$ & [Fe/H] & $\sigma_{\rm [Fe/H]}^{\rm rel}$ & $\sigma_{\rm [Fe/H]}^{\rm abs}$ & $\xi$ & $\sigma_\xi^{\rm rel}$ & $\sigma_\xi^{\rm abs}$ &  $\log\epsilon_{\rm C}$ & $\sigma_{\log\epsilon_{\rm C}}^{\rm rel}$ & $\sigma_{\log\epsilon_{\rm C}}^{\rm abs}$  & [C/Fe] & $\sigma_{\rm [C/Fe]}^{\rm rel}$ & $\sigma_{\rm [C/Fe]}^{\rm abs}$ & N & N3 & \ldots \\    
 & & [K] & & [cm s$^{-2}$] & & & & & & [km s$^{-1}$] & & &  &  & & & & & & & \ldots \\    
\hline 
  CS~22175-007      &	   31 &	5108 &	100 & 2.46&  0.26 & 0.36 & $-2.81$ &  0.13 & 0.18&  1.67&  0.14&  0.24 &     5.77 & 0.19 & 0.26 & $   0.19$ &  0.18&  0.27&   1 & 1 & $\ldots$ \\	
  CS~22186-023      &	   55 &	5066 &	100 & 2.19&  0.24 & 0.34 & $-2.72$ &  0.13 & 0.18&  1.58&  0.11&  0.21 &     5.97 & 0.19 & 0.25 & $   0.30$ &  0.18&  0.27&   1 & 1 & $\ldots$ \\	
  CS~22186-025      &	   32 &	4985 &	100 & 1.70&  0.26 & 0.36 & $-2.87$ &  0.14 & 0.19&  2.14&  0.13&  0.23 &     4.83 & 0.20 & 0.27 & $  -0.68$ &  0.19&  0.29&   1 & 1 & $\ldots$ \\	
  CS~22886-042      &	   39 &	4881 &	100 & 1.85&  0.25 & 0.35 & $-2.68$ &  0.12 & 0.18&  1.84&  0.12&  0.22 &     5.72 & 0.19 & 0.26 & $   0.01$ &  0.19&  0.28&   1 & 1 & $\ldots$ \\	
  CS~22892-052      &	   46 &	4884 &	100 & 1.81&  0.26 & 0.36 & $-2.95$ &  0.14 & 0.19&  1.67&  0.12&  0.22 &     6.44 & 0.19 & 0.26 & $   1.00$ &  0.18&  0.28&   1 & 1 & $\ldots$ \\	
  CS~22945-028      &	   31 &	5126 &	100 & 2.55&  0.26 & 0.36 & $-2.66$ &  0.13 & 0.18&  1.53&  0.14&  0.24 &     5.93 & 0.19 & 0.26 & $   0.21$ &  0.18&  0.27&   1 & 1 & $\ldots$ \\	
  CS~22957-013      &	   35 &	4904 &	100 & 1.96&  0.25 & 0.35 & $-2.64$ &  0.14 & 0.19&  1.79&  0.12&  0.22 &     5.85 & 0.19 & 0.26 & $   0.10$ &  0.17&  0.27&   1 & 1 & $\ldots$ \\	
  CS~22958-083      &	   32 &	5101 &	100 & 2.40&  0.26 & 0.36 & $-2.79$ &  0.12 & 0.18&  1.50&  0.13&  0.23 &     6.24 & 0.20 & 0.26 & $   0.64$ &  0.18&  0.27&   1 & 1 & $\ldots$ \\	
  CS~22960-010      &	   35 &	5737 &	100 & 4.85&  0.25 & 0.35 & $-2.65$ &  0.12 & 0.17&  1.53&  0.17&  0.27 &     6.56 & 0.17 & 0.24 & $   0.82$ &  0.16&  0.25&   1 & 1 & $\ldots$ \\	
  CS~29491-069      &	   57 &	5103 &	100 & 2.45&  0.24 & 0.34 & $-2.81$ &  0.13 & 0.18&  1.54&  0.12&  0.22 &     5.76 & 0.19 & 0.25 & $   0.18$ &  0.17&  0.27&   1 & 1 & $\ldots$ \\	
$\vdots$  &$\vdots$  &$\vdots$  &$\vdots$  &$\vdots$  &$\vdots$  & $\vdots$ & $\vdots$ & $\vdots$ & $\vdots$ & $\vdots$ & $\vdots$ & $\vdots$ & $\vdots$ & $\vdots$ & $\vdots$ &  $\vdots$ & $\vdots$& $\vdots$ &  $\vdots$& $\vdots$ &$\ldots$ \\ 
  HE~2338-1618      &	   40 &	5515 &	100 & 3.38&  0.27 & 0.37 & $-2.65$ &  0.12 & 0.18&  1.43&  0.16&  0.26 &     6.22 & 0.18 & 0.25 & $   0.47$ &  0.18&  0.27&   1 & 1 & $\ldots$ \\	
  HE~2345-1919      &	   44 &	5617 &	100 & 4.46&  0.25 & 0.35 & $-2.46$ &  0.12 & 0.18&  1.47&  0.16&  0.26 &     6.17 & 0.19 & 0.24 & $   0.24$ &  0.17&  0.26&   1 & 1 & $\ldots$ \\	
  HE~2347-1254      &	   80 &	6132 &	100 & 3.95&  0.24 & 0.34 & $-1.83$ &  0.13 & 0.18&  1.67&  0.12&  0.22 &     6.83 & 0.15 & 0.22 & $   0.27$ &  0.16&  0.26&   1 & 1 & $\ldots$ \\	
  HE~2347-1334      &	   81 &	4453 &	100 & 0.95&  0.24 & 0.34 & $-2.55$ &  0.12 & 0.19&  2.38&  0.11&  0.21 &     5.33 & 0.21 & 0.26 & $  -0.50$ &  0.18&  0.27&   1 & 1 & $\ldots$ \\	
  HE~2347-1448      &	   43 &	6162 &	100 & 3.98&  0.27 & 0.37 & $-2.31$ &  0.12 & 0.18&  0.84&  0.17&  0.27 &     6.58 & 0.18 & 0.24 & $   0.50$ &  0.19&  0.27&   1 & 1 & $\ldots$ \\	
\hline
\end{tabular}
\end{table}