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Home All issues Volume 506 / No 1 (October IV 2009) A&A, 506 1 (2009) 385-389 Full HTML
 

 

Table 1:

Transiting Exoplanets characteristics.
  Planet Star
Object M($M_{\rm J}$) R($R_{\rm J}$) Period a(au) log ( $F_{\rm inc}$) e i Spec. Type $T_{\rm eff}(K)$ Age(Gyr) M($M_\odot$) [Fe/H] R($R_{\odot}$)
CoRoT-1ba $1.03\pm0.12$ $1.49\pm0.08$ 1.50 0.0254 9.467 - 85.1 G0V 5950 0.2-4 0.95 -0.3 1.11
CoRoT-2bb $3.31\pm0.16$ $1.465\pm0.029$ 1.74 0.0281 9.102 - 87.84 K0V 5625 0.2-4 $0.97\pm0.06$   0.902
CoRoT-3bc $21.66\pm1.0$ $1.01\pm0.07$ 4.25 0.057 9.277 - 85.9 F3V 6740 1.6-2.8 1.37 -0.02 1.56
CoRoT-4bd $0.72\pm0.08$ 1.19+0.06-0.05 9.20 0.09 8.468 - 90 F0V 6190 1.+1.0-0.3 1.1   1.15
HAT-P-2be $8.04\pm 0.40$ $0.98\pm0.04$ 5.63 0.0677 8.962 0.5163 90 F8 6290 $2.7\pm1.4$ 1.31 0.12 1.48
a Barge et al. (2008), b Alonso et al. (2008), c Deleuil et al. (2008), d Moutou et al. (2008), e Winn et al. (2007).
For all the CoRoT objects, e=0 is assumed in the analysis of the light-curve and of the radial velocity data.

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