\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}