\begin{table}%t4
\caption{\label{tab4}Elemental abundances and $^{12}$C/$^{13}$C ratios for CEMP stars.}
\small%\centerline
{
\begin{tabular}{lllllllllllll}
\hline
\hline
Star         & \teff & \logg & [Fe/H]  & [C/Fe]& [O/Fe] & [N/Fe] & [Mg/Fe] & 
[Sr/Fe] &  [Ba/Fe] & $^{12}$C/$^{13}$C & $A$(Li) &  Ref \\
\hline
\noalign{\smallskip}
{\bf CEMP-no stars$^{a}$} \\
\noalign{\smallskip} 
CS~22877-001 & 5100 &  2.2 &   $-$2.71 & +1.0  & \nodata& +0.0   & +0.29    & $-
$0.12 & $-$0.49 & $>$10 &  \nodata&    4 \\
CS~22949-037 & 4900 &  1.7 &   $-$3.79 & +1.17 & +1.98  & +2.57  & +1.56    &  
+0.33  & $-$0.58 &    4  &  \nodata&   10,17 \\
CS~22957-027 & 5100 &  1.4 &   $-$3.11 & +2.37 & \nodata& +1.62  & +0.69    & $-
$0.56 & $-$1.23 &    8  &  \nodata&   3,19 \\
CS~22958-042 & 6250 &  3.5 &   $-$2.85 & +3.15 & +1.12  & +2.15  & +0.32    & $-
$0.2  & $<$$-$0.53 &  9  &  $<$$0.6$&   TP \\
CS~29498-043 & 4600 &  1.2 &   $-$3.53 & +2.09 & +2.43  & +2.27  & +1.75    & $-
$0.47 & $-$0.46 &    6  &  \nodata&   3,7 \\
CS~29502-092 & 5000 &  2.1 &   $-$2.77 & +1.0  & \nodata& +1.0   & +0.37    & $-
$0.40 & $-$0.82 &  ~20  &  \nodata&    4 \\
G~77-61      & 4000 &  5.0 &   $-$4.0  & +3.2  & +2.2   & +2.2   & +0.49    & 
\nodata & \nodata & 5     &   $<$1.0&    18 \\
HE~0007-1832 & 6515 &  3.8 &   $-$2.65 & +2.55 & \nodata& +1.85  & \nodata  & 
\nodata & +0.16   & 10  &  \nodata&    9 \\
HE~0107-5240 & 5180 &  2.2 &   $-$5.3  & +4.1  & \nodata& +2.3   & \nodata  & 
\nodata & \nodata &\nodata&  \nodata&    8 \\
HE~1327-2326 & 6180 &  3.7 &   $-$5.6  & +4.1  & 2.8    & +4.5   & \nodata  &   
+1.1  & $<+1.5$ &\nodata&  $<$1.5&    11,11a,21 \\
\noalign{\smallskip} 
{\bf CEMP-no/s stars$^{b}$}  \\
\noalign{\smallskip} 
CS~29528-041 & 6166 &  4.0 &   $-$3.30 & +1.59 & $<$1.40& +3.07  & +0.4     & $-
$0.2  & +0.97   &\nodata&    1.71 &    TP \\
CS~31080-095 & 6100 &  4.5 &   $-$2.85  & +2.69 & 2.23  & +0.70  & +0.65    & $-
$0.41 & +0.77   & $>$40&    1.73 &    TP \\
\noalign{\smallskip} 
{\bf CEMP-s stars$^{c}$}  \\
\noalign{\smallskip}  
CS~22880-074 & 5850 &  3.8 &   $-$1.93 & +1.3  & \nodata& $-$0.1 &  \nodata &  
+0.39  & +1.31   & $>$40 &  \nodata&   3,19 \\
CS~22942-019 & 5000 &  2.4 &   $-$2.64 & +2.0  & \nodata& +0.3   &  \nodata &  
+1.7   & +1.92   &  8    &  \nodata&   3,19 \\
CS~30301-015 & 4750 &  0.8 &   $-$2.64 & +1.6  & \nodata& +0.6   &  \nodata &  
+0.3   & +1.45   &  6    &  \nodata&   3 \\
 \noalign{\smallskip} 
{\bf CEMP-r/s stars$^{d}$}  \\
  \noalign{\smallskip} 
CS~22898-027 & 6250 &  3.7 &   $-$2.26 & +2.2  & \nodata& +0.9   &  \nodata &  
+0.92  & +2.23   & $>$20 &    2.10 &   3,19 \\
CS~22948-027 & 4600 &  1.0 &   $-$2.57 & +2.43 & \nodata& +1.75  & +0.31    &  
+0.90  & +2.26   &  10   &    0.30 &   3,19 \\
CS~29497-030 & 6650 &  3.5 &   $-$2.70 & +2.38 & +1.67  & +1.88  & +0.64    &  
+0.84  & +2.17   &  $>$10&   $<$1.10 &   20 \\
             & 7000 &  4.1 &   $-$2.57 & +2.30 & +1.48  & +2.12  & +0.44    &  
+1.34  & +2.32   & \nodata &   \nodata &   13 \\
CS~29497-034 & 4800 &  1.8 &   $-$2.90 & +2.63 & \nodata& +2.38  & +0.72    &  
+1.00  & +2.03   &  12   &    0.10 &   12 \\
CS~29526-110 & 6500 &  3.2 &   $-$2.38 & +2.2  & \nodata& +1.4   &  \nodata &  
+0.88  & +2.11   &\nodata&  \nodata &   5    \\
CS~31062-012 & 5600 &  3.0 &   $-$2.55 & +2.1  & \nodata& +1.2   &  \nodata &  
+0.30  & +1.98   &  8    &  \nodata&   3,6 \\
CS~31062-050 & 5600 &  3.0 &   $-$2.33 & +2.0  & \nodata& +1.2   & +0.84    &  
+0.91  & +2.80   &  8    &  \nodata&   3,6 \\
HE~0024-2523 & 6625 &  4.3 &   $-$2.67 & +2.6  & +0.40  & +2.1   & +0.73    &  
+0.34  & +1.46   &  6    &    1.50 &   15 \\
LP~625-44    & 5500 &  2.8 &   $-$2.71 & +2.1  & \nodata& +1.0   &  \nodata &  
+1.15  & +2.74   &  20   &    0.40 &   1,2 \\
LP~706-7     & 6250 &  4.5 &   $-$2.74 & +2.15 & \nodata& +1.80  &  \nodata &  
+0.15  & +2.01   & $>$15 &    2.09 &   3,16 \\
HE~0143-0441 & 6370 &  4.4 &   $-$2.16 & +1.66 & \nodata& $-$0.04&  \nodata 
&\nodata  & +2.31   & 10    &  \nodata &   9 \\
HE~0338-3945 & 6160 &  4.1 &   $-$2.42 & +2.13 & +1.40  & +1.55  &  +0.30   &  
+0.74  & +2.41   &10     &  \nodata &   14 \\
HE~2148-1247 & 6380 &  4.3 &   $-$2.3  & +1.91 & \nodata& +1.65  &  \nodata & 
\nodata & +2.36   & 10    &  \nodata&   9 \\
\hline
\end{tabular}}
\smallskip
$^{a}$[C/Fe$] > +1.0$ and [Ba/Fe] $<$ 0.0 (Beers \& Christlieb \cite{Beers2005});
$^{b}$[C/Fe$] > +1.0$ and $+0.5 < {\rm [Ba/Fe]} < +1.0$ ;
$^{c}$[C/Fe$] > +1.0$, [Ba/Fe] $>$ +1.0, and [Ba/Eu$] > +0.5$ (Beers \& 
Christlieb \cite{Beers2005});
$^{d}$[C/Fe$] > +1.0$ and $0.0 < {\rm [Ba/Fe]} < +0.5$ (Beers \& Christlieb 
\cite{Beers2005}).\\
Ref.:
(1) Aoki et~al. (\cite{Aoki2000});
(2) Aoki et~al. (\cite{Aoki2001});
(3) Aoki et~al. (\cite{Aoki2002a});
(4) Aoki et~al. (\cite{Aoki2002b});
(5) Aoki et~al. (\cite{Aoki2002c});
(6) Aoki et~al. (\cite{Aoki2003});
(7) Aoki et~al. (\cite{Aoki2004});
(8) Christlieb et~al. (\cite{Christlieb2002});
(9) Cohen et~al. (\cite{Cohen2003});
(10) Depagne et~al. (\cite{Depagne2002});
(11) Frebel et~al. (\cite{Frebel2005});
(11a)Frebel et~al. (\cite{Frebel2006});
(12) Hill et~al. (\cite{Hill2000});
(13) Ivans et~al. (\cite{Ivans2005});
(14) Jonsell et~al. (\cite{Jonsell2006});
(15) Lucatello et~al. (\cite{Lucatello2003});
(16) Norris et~al. (1997);
(17) Norris et~al. (\cite{Norris2002});
(18) Plez et~al. (\cite{Plez2005e});
(19) Preston \& Sneden (\cite{Preston2001});
(20) Sivarani et~al. (\cite{Sivarani2004});
(21) Aoki et~al. (\cite{Aoki2006b});
(TP) This paper. 
\end{table}