\begin{table}
%\centering
\par
\caption{\label{t:data}Typical example (all C-stars) for the And~II results, extracted from the full table (with 2307 entries), which is available via CDS. Column 1 gives an ID code, Col. 2 the aprox. 4-digit $xy$-coordinates on CCD) for every star, while Cols. 3 and 4 list
the coordinates (J2000.0) in the form {\tt hhmmss.sss} and {\tt ddmmss.ss},
respectively. A special flag {\tt F} is given in Col. 4, which 
denotes in which region of Fig.~\ref{figure3} the star falls ({\tt c}
for carbon stars, {\tt o} for oxygen-rich stars, {\tt r} for the rest), if it is member of
\textit{sample~2}. If the flag {\tt F} is {\tt u} (for unclassified), the star is from
\textit{sample~1} and not included in the smaller \textit{sample~2}, which means it has
only $Vi$-photometry. Columns~\mbox{5--7} list the photometric results, {\tt i},
{\tt V-i}, {\tt TiO-CN}. The astrometric data may be afflicted with a systematic
error of 0.5--1.2$\arcsec$ introduced by the accuracy limits of the GSC reference
stars (Taff et~al. \cite{TLBGM90}), the mean uncertainty of the MIDAS
astrometric solution is 0.05$\arcsec$ rms (with a maximum of 0.11$\arcsec$). } 
\par
\begin{small}
\begin{verbatim}
ID Pixel    RA         DE        F i      V-i  TiO-CN  
C1 12381204 011627.57  332530.15 c 20.56  2.21  -0.57
C2 11790863 011628.39  332426.30 c 20.35  1.76  -0.58
C3 11731832 011628.69  332727.74 c 19.98  2.15  -0.63
C3 09161842 011632.53  332729.53 c 19.67  2.14  -0.55
C4 08451648 011633.55  332653.10 c 19.17  2.07  -0.54
C5 04671813 011639.23  332723.67 c 19.42  2.24  -0.51
C6 01920617 011643.19  332337.96 c 20.08  2.88  -0.52
.        .          .         . .      .     .
.        .          .         . .      .     .
\end{verbatim}
\end{small}
\end{table}