\begin{table}
 %\centering
\par
\caption {\label{classification} Classical T Tauri stars that belong to NGC~2264 and were observed by CoRoT.}
\begin{tabular}{llllllllllll}
\hline\hline
\noalign{\smallskip}
RA        & Dec      & $V$     & CoRoT ID  & \hal {\it EW} & UV1    & UV2    & \hal10\% & SpT & LC group & Period & $\alpha_{\rm IRAC}$\\
(deg)     & (deg)    & (mag) &           & (\AA)   & (mag)  & (mag)  &          &     &          & (days) &       \\  
\hline
 99.89338 &  9.91424 & 16.64 & 223957455 & 22.1    & ...    &  ...   & x        & ... & NP       & ...    & ...   \\
 99.92281 &  9.77214 & 14.64 & 223959618 & 28.4    & ...    &  ...   & x        & ... & PII      & 3.87   & ...   \\
 99.99684 &  9.45681 & 16.34 & 223964667 & 42.2    & ...    &  ...   & x        & ... & PII      & 6.45   & --1.87 \\
100.04666 &  9.63501 & 16.67 & 223968039 & 52.9    & --1.15  &  ...   & x        & K6  & NP       & ...    & --1.35 \\
100.05673 &  9.41375 & 13.02 & 223968688 & 0.60    & ...    &  ...   & x        & K0  & PI       & 1.11   & --2.81 \\ 
100.05710 &  9.94183 & 17.02 & 400007614 & 130.2   & ...    &  ...   & x        & M2  & NP       & ...    & 0.0149\\
100.09620 &  9.46176 & 16.04 & 223971231 & 49.5    & --1.62  &  ...   & x        & K5  & NP       & ...    & --1.73 \\        
100.09889 &  9.92330 & 17.55 & 223971383 & 80.6    & ...    &  ...   & x        & ... & PI       & 4.66   & --1.22 \\
100.12006 &  9.51718 & 15.20 & 223972652 & 39.1    & --0.89  &  ...   & ...      & K4  & NP       & ...    & --0.56 \\
100.12186 &  9.73542 & 17.69 & 400007809 & 31.3    & --1.36  &  ...   & x        & M2  & NP       & ...    & ...   \\
100.12859 &  9.57794 & 16.03 & 223973200 & 22.2    & ...    &  ...   & x        & K1  & NP       & ...    & --1.29 \\        
100.13013 &  9.51864 & 15.43 & 223973292 &  1.7    & --0.91  &  ...   & ...      & K6  & PI       & 1.96   & ...   \\         
100.15217 &  9.84601 & 16.67 & 400007538 & 21.1    & --2.11  & --1.687 & ...      & M2  & NP       & ...    & --1.29 \\ 
100.15262 &  9.80638 & 15.62 & 500007298 &  4.9    & --1.43  & --0.606 & ...      & K5  & PI       & 15.70  & --4.19 \\
100.15781 &  9.58167 & 16.64 & 400007528 & 23.4    & ...    &  ...   & x        & M3  & NP       & ...    & --1.87 \\ 
100.16297 &  9.84961 & 15.43 & 500007252 & 46.5    & --1.89  &  ...   & x        & K4  & PII      & 7.06   & --1.55 \\
100.16840 &  9.84735 & 15.50 & 500007272 & 58.3    & ...    &  ...   & ...      & K7  & PI       & 3.76   & --2.42 \\
100.17086 &  9.46509 & 16.53 & 500007505 & 13.2    & ...    &  ...   & ...      & ... & NP       & ...    & --1.97 \\
100.17095 &  9.79936 & 16.01 & 500007379 &  7.5    & --1.22  & --0.984 & ...      & K7  & PI       & 14.15  & --1.97 \\
100.17216 &  9.85066 & 15.70 & 500007315 & 24.5    & --2.13  &  ...   & ...      & K7  & PII      & 7.80   & --1.19 \\
100.17233 &  9.90385 & 13.57 & 223975844 & 12.2    &  0.02  &  ...   & x        & G3  & PI       & 3.31   & ...   \\        
100.17435 &  9.86237 & 15.49 & 500007269 & 23.4    & ...    &  ...   & ...      & K5  & PI       & 3.75   & --1.53 \\
100.17576 &  9.56040 & 12.09 & 223976028 &  7.3    & ...    &  ...   & x        & G0  & NP       & ...    & --1.12 \\
100.18006 &  9.78535 & 16.33 & 500007460 & 27.1    & ...    &  ...   & x        & K6  & NP       & ...    & ...   \\
100.18580 &  9.54061 & 18.13 & 500007930 & 60.0    & ...    &  ...   & ...      & M3  & NP       & ...    & --2.61 \\
100.18819 &  9.47901 & 14.55 & 223976747 &  7.2    & --0.16  &  ...   & x        & K2  & PII      & 3.16   & ...   \\
100.19793 &  9.82471 & 14.14 & 500007120 & 12.8    & ...    & --0.806 & x        & K1  & PII      & 4.23   & --1.41 \\
100.19968 &  9.55087 & 18.24 & 500007963 & ...     & ...    & --0.917 & ...      & ... & PI       & 2.56   & ...   \\  
100.20505 &  9.96077 & 17.46 & 500007730 & 50.8    & ...    &  ...   & ...      & M1  & PI       & 11.85  & --2.67 \\
100.20789 &  9.61375 & 15.37 & 223977953 & 66.3    & --1.79  & -1.906 & ...      & K4  & PII      & 4.96   & --1.43 \\        
100.21081 &  9.91593 & 15.13 & 500007209 & 11.2    & ...    &  ...   & x        & K2  & PII      & 2.51   & --2.14 \\
100.21326 &  9.74615 & 12.05 & 223978308 &  3.5    & ...    &  ...   & x        & G0  & PII      & 5.40   & --1.69 \\
100.22346 &  9.55686 & 14.70 & 223978921 & 18.2    & ...    & --0.643 & x        & K1  & NP       & ...    & --2.29 \\
100.22607 &  9.82232 & 16.39 & 500007473 & 161.1   & --2.11  &  ...   & x        & M0  & NP       & ...    & --0.38 \\
100.22990 &  9.84718 & 15.89 & 500007354 &  2.8    & --0.64  & --0.774 & ...      & K5.5 & PI      & 1.17   & --9.15 \\
100.23215 &  9.85385 & 15.54 & 500007283 & 8.00    & ...    &  ...   & ...      & K5.5 & PI      & 3.23   & --0.29 \\
100.23663 &  9.63029 & 15.09 & 223979728 & 113.2   & ...    & --1.353 & x        & M1  & NP       & ...    & --1.17 \\
100.24208 &  9.61483 & 18.05 & 223980048 & 34.0    & ...    &  ...   & ...      & ... & PII      & 4.06   & --1.41 \\
100.24447 &  9.60368 & 17.40 & 223980233 & 22.2    & ...    &  ...   & ...      & M4  & NP       & ...    & ...   \\
100.24510 &  9.65522 & 17.02 & 223980258 &  27.9   & ...    &  ...   & x        & M0  & PI       & 7.05   & --1.39 \\
100.24516 &  9.51592 & 14.04 & 223980264 & 14.3    & ...    &  ...   & x        & K2.5 & PII      & 3.46   & --1.51 \\
100.24770 &  9.99596 & 15.34 & 223980412 & 7.41    & --0.53  &  ...   & ...      & K5  & PI       & 3.23   & ...   \\
100.24792 &  9.49770 & 17.00 & 500007610 & 26.2    & ...    &  ...   & ...      & M3  & PII      & 4.66   & --1.16 \\
100.24811 &  9.58636 & 15.58 & 223980447 &  6.4    & --1.01  & --0.427 & x        & K6  & PI       & 1.67   & --1.14 \\
100.25209 &  9.75088 & 15.39 & 223980688 & 15.0    & --0.59  & --0.723 & x        & K3  & PII      & 4.16   & --2.10 \\
100.25214 &  9.48776 & 14.56 & 223980693 & 16.6    & ...    &  ...   & x        & K4  & PII      & 5.35   & --1.72 \\
100.25323 &  9.85620 & 14.63 & 500007157 &  1.6    & ...    & --0.658 & ...      & K1  & PI       & 4.36   & ...   \\
100.25408 &  9.54568 & 13.51 & 223980807 &  6.4    & ...    &  ...   & x        & K1  & NP       & ...    & --1.56 \\  
100.25767 &  9.64475 & 14.70 & 223981023 &  1.5    & ...    &  ...   & x        & K4  & PII      & 7.05   & --2.41 \\
100.26266 &  9.62660 & 19.17 & 500008211 & 34.1    & ...    &  ...   & ...      & M1  & NP       & ...    & --1.22 \\
100.26503 &  9.50806 & 17.67 & 400007803 & 20.4    & ...    &  ...   & ...      & ... & PII      & 9.75   & --1.12 \\
100.26789 &  9.41449 & 15.79 & 500007335 & 101.8   & --2.34  &  ...   & x        & M0  & PII      & 7.36   & --0.97 \\
100.26905 &  9.64190 & 17.88 & 500007857 & 108.    & ...    &  ...   & ...      & M3  & NP       & ...    & --0.78 \\
100.27071 &  9.84613 & 14.36 & 223981811 & 36.5    & --0.29  & --0.816 & x        & K1  & PII      & 3.73   & --1.91 \\
100.27124 &  9.86239 & 15.39 & 500007248 &  1.7    & --0.75  & --0.570 & ...      & K5  & PI       & 1.88   & --3.06 \\
100.27583 &  9.60638 & 13.52 & 223982136 & 10.0    & ...    &  ...   & x        & G3  & PI       & 3.01   & --2.03 \\
100.27595 &  9.41769 & 18.01 & 500007896 & 34.7    & ...    &  ...   & ...      & M5  & PI       & 9.30   & --1.58 \\
100.27679 &  9.47745 & 17.30 & 400007686 &  56.1   & ...    &  ...   & x        & M1.5 & NP      & ...    & --1.57 \\
100.27808 &  9.57943 & 15.97 & 500007369 & 49.4    & ...    &  ...   & x        & G6  & NP       & ...    & ...   \\      
100.28734 &  9.56278 & 17.53 & 500007752 &  51.0   & ...    &  ...   & x        & M3  & PI       & 4.01   & --0.88 \\
100.29582 &  9.59881 & 17.44 & 500007727 & 61.5    & ...    & --2.037 & x        & K7  & NP       & ...    & --0.93 \\
100.30241 &  9.87533 & 14.07 & 500007115 & 35.3    & ...    &  ...   & x        & G   & PII      & 2.01   & --1.72 \\
100.30362 &  9.43746 & 13.76 & 500007089 & 85.6    & ...    &  ...   & x        & K4  & NP       & ...    & --1.33 \\
100.31035 &  9.62065 & 17.23 & 500007667 &  4.1    & ...    & --0.697 & ...      & ... & PI       & 5.41   & --2.96 \\
100.32188 &  9.90899 & 15.64 & 223985009 & 58.3    & --2.40  &  ...   & ...      & K7  & NP       & ...    & ...   \\
\hline
100.32467 &  9.48364 & 18.55 & 500008049 & 231.4   & ...    &  ...   & ...      & M2.5 & NP      & ...    & --0.68 \\
100.32534 &  9.64038 & 18.58 & 500008061 & 32.5    & ...    &  ...   & ...      & M3  & PI       & 0.98   & --2.89 \\
100.32613 &  9.56488 & 15.02 & 223985261 & 28.9    & --0.97  &  ...   & x        & K4  & NP       & ...    & --2.39 \\
100.33752 &  9.56005 & 15.20 & 223985987 & 10.6    & ...    &  ...   & x        & K6  & PII      & 3.31   & --1.44 \\
100.34851 &  9.78788 & 17.93 & 500007872 &  5.2    & ...    & --0.767 & ...      & ... & PI       & 8.20   & --2.01 \\
100.35227 &  9.62653 & 17.38 & 400007709 &  8.9    & --0.99  &  ...   & ...      & M3  & PI       & 0.76   & ...   \\
100.35677 &  9.57861 & 16.15 & 223987178 & 15.9    & --0.61  & --1.233 & ...      & M0  & PII      & 4.96   & --1.11 \\
100.36250 &  9.50365 & 17.47 & 400007734 & 25.8    & ...    &  ...   & ...      & M1  & NP       & ...    & --1.88 \\
100.37968 &  9.44951 & 14.19 & 500007122 & 25.9    & ...    &  ...   & x        & ... & PII      & 12.53  & --1.44 \\
100.38169 &  9.80912 & 14.63 & 223988742 & 5.16    & --0.08  & --0.409 & ...      & K2  & PI       & 5.03   & --2.84 \\
100.38331 &  10.0068 & 15.59 & 223988827 & 13.1    & ...    &  ...   & ...      & K5  & PI       & 4.78   & --2.69 \\
100.38543 &  9.63540 & 14.66 & 223988965 &  1.3    & --0.67  &  ...   & ...      & K6  & PI       & 3.23   & --2.83 \\
100.39397 &  9.60904 & 17.16 & 223989567 &  4.5    & --0.83  &  ...   & x        & M1  & NP       & ...    & ...   \\
100.40536 &  9.75186 & 15.44 & 223990299 & 35.0    & ...    & --0.826 & x        & K4  & PI       & 4.51   & --0.93 \\
100.41155 &  9.53661 & 15.40 & 500007249 & 58.6    & ...    &  ...   & x        & K4  & NP       & ...    & --1.55 \\ 
100.41564 &  9.67443 & 13.86 & 223990964 & 52.5    & ...    & --1.061 & ...      & K4  & NP       & ...    & --1.46 \\ 
100.42867 &  9.41900 & 16.65 & 223991832 & 75.8    & ...    &  ...   & x        & ... & PII      & 8.40   & --1.38 \\
100.47104 &  9.96747 & 14.99 & 223994721 &  9.5    & ...    &  ...   & x        & K7  & NP       & ...    & --1.47 \\
\hline
\end{tabular}
\tablefoot {The \hal \ equivalent widths come from \citet{reb02} and \citet{dah05}, except for
six stars (CID~223957455, 223959618, 223964667, 223968688, 223991832, 223994721)
for which we measured the \hal \ equivalent width ourselves, using the high
resolution hectoechelle spectra kindly provided by Gabor F{\H u}r{\'e}sz. The $U-V$ excesses
were taken from \citet{reb02} (UV1) and \citet{fal06} (UV2, the $U-V$ excess data table was provided by Cassandra
Fallscheer). Stars that have an
\hal \ width at~10\% intensity larger than $270$~\kms \ are identified by a x sign
in column eight, following the classification of \citet{fur06}. The LC group
and period values were determined in the present work. The $\alpha_{\rm IRAC}$ index
is described in Sect.~\ref{corot_spitzer} and comes from \citet{tei08}.}
\end{table}