\begin{table}%t14
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\par
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%\caption {\label{solutions}Status of transit candidate resolution following the analysis of complementary observations.}
%%\centerline {\tiny \begin{tabular}{lllllll}
%\hline  \hline
%CoRoT-ID &WinID &Depth &CoRoT P$^a$ &Nature& K &RV P\\
%         &      &\%  &  [d] &       &[km~s$^{-1}$]& [d]\\ 
%\hline
%102723949& E1-2046& 1.17& 50.2$^b$ &SB2 &$>$15& -- \\ 
%102874481& E2-3010& 1.72& 23.2 &SB2& $>$17& -- \\ 
%102805893& E2-3854& 0.136& 1.14 &SB2& 43& -- \\ 
%102954464& E2-3856& 2.05& 16.56& SB1& 60& -- \\ 
%102763847& E1-1158& 1.36& 10.53 &SB1& 25& -- \\ 
%102825481 & E2-0203 & 3.43 & 5.168 & SB1 & 16.9 & --\\
%102815260& E2-2430& 1.16& 3.587 &SB1& 23.5& -- \\ 
%102829121& E1-0399& 1.5 &33.06 &SB1 &20.5&-- \\ 
%102855534& E2-1736& 1.18& 21.72 &SB1& 15.5& -- \\ 
%102912369& E2-2604& 0.25 &3.82 &aperture BEB& -- &-- \\ 
%102753331& E2-1136& 0.17& 1.22 & aperture BEB &-- &-- \\ 
%102802430& E2-4300 & 0.51 & 5.806 & aperture BEB & -- & --\\
%102815260& E1-0288& 0.37 &7.89 & aperture BEB& -- &-- \\ 
%102802996& E2-3425& 0.36& 1.185& aperture BEB& --& -- \\ 
%102798247& E2-1857& 0.47 &0.822&unresolved BEB &6.3& 8.734 \\ 
%102788073& E2-2009& 0.41 &10.85& unresolved BEB &-- &21.69 \\ 
%102869286& E1-2329& 0.37& 1.867& unresolved BEB& -- &3.734 \\ 
%102876631 &E1-3336& 0.17& 1.389& unresolved BEB& --& -- \\ 
%102855472& E2-0704&0.72 &2.15& unresolved BEB & &  \\
%102753331 &E1-4617& 4.0 &19.76 &hot/fast star& -- &-- \\ 
%102895957& E1-0783& 0.64& $>$32& hot/fast star& --& -- \\ 
%102940315& E2-4467& 1.4 &16.45 &hot/fast star& -- &-- \\ 
%102806520& E1-4591 &0.29 &4.295 &hot/fast star& --& -- \\ 
%102874481& E2-1677& 3.0 &$>$33& hot/fast star & &\\
%102826302& E2-1712& 0.24 &2.767& unknown& --& -- \\ 
%102780627& E1-4998& 1.9 &10.08 &unknown & $>$23& -- \\ 
%102779966& E1-4108 & 0.5 & 7.366 & unknown & $<$0.02 & -- \\
%102890318& E2-1126& 2.16 &1.509& planet& 0.188& -- \\ 
%102912369& E1-0330& 1.2 &9.202& planet &0.063& --\\ 
%\hline
%\end{tabular}}
%$^a$  {for a more accurate determination of CoRoT period, see Paper~I.}
%$^b$~{The period of this candidate was not measured during IRa01, but was inferred after it was re-observed by CoRoT during LRa01 at the end of 2008.}
%\end{table}