Table 14:

Status of transit candidate resolution following the analysis of complementary observations.
WinID Depth CoRoT Pa Nature K RV P  
    % [d]   [km s-1] [d]
E1-2046 1.17 50.2b SB2 >15 -  
E2-3010 1.72 23.2 SB2 >17 -  
E2-3854 0.136 1.14 SB2 43 -  
E2-3856 2.05 16.56 SB1 60 -  
E1-1158 1.36 10.53 SB1 25 -  
E2-0203 3.43 5.168 SB1 16.9 -  
E2-2430 1.16 3.587 SB1 23.5 -  
E1-0399 1.5 33.06 SB1 20.5 -  
E2-1736 1.18 21.72 SB1 15.5 -  
E2-2604 0.25 3.82 aperture BEB - -  
E2-1136 0.17 1.22 aperture BEB - -  
E2-4300 0.51 5.806 aperture BEB - -  
E1-0288 0.37 7.89 aperture BEB - -  
E2-3425 0.36 1.185 aperture BEB - -  
E2-1857 0.47 0.822 unresolved BEB 6.3 8.734  
E2-2009 0.41 10.85 unresolved BEB - 21.69  
E1-2329 0.37 1.867 unresolved BEB - 3.734  
E1-3336 0.17 1.389 unresolved BEB - -  
E2-0704 0.72 2.15 unresolved BEB      
E1-4617 4.0 19.76 hot/fast star - -  
E1-0783 0.64 >32 hot/fast star - -  
E2-4467 1.4 16.45 hot/fast star - -  
E1-4591 0.29 4.295 hot/fast star - -  
E2-1677 3.0 >33 hot/fast star      
E2-1712 0.24 2.767 unknown - -  
E1-4998 1.9 10.08 unknown >23 -  
E1-4108 0.5 7.366 unknown <0.02 -  
E2-1126 2.16 1.509 planet 0.188 -  
E1-0330 1.2 9.202 planet 0.063 -  
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.

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