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Table 1:

Stellar/planetary parameters of CoRoT-2a/b.
Stara Value $\pm$ Error Ref.b
$P_{\rm s}$ $(4.522 ~ \pm ~ 0.024)$ d L09
$P_{\rm s}^*$ 4.57 d  
Spectral type G7V B08
Planetc Value $\pm$ Error Ref.
$P_{\rm p}$ $(1.7429964 ~ \pm ~ 0.0000017)$ d A08
$T_{\rm c}$ [BJD] $(2~454~237.53362 ~ \pm ~ 0.00014)$ d A08
i $(87.7 ~ \pm ~ 0.2)$ C09
$R_{\rm p}/R_{\rm s}$ $(0.172 ~ \pm ~ 0.001)$ C09
$a/R_{\rm s}$ $(6.70 ~ \pm ~ 0.03)$ A08
ua, ub $(0.41\pm0.03),~ (0.06\pm 0.03)$ A08

a $P_{\rm s}$ - stellar rotation period, $P_{\rm s}^*$ - stellar rotation period used for the observation interval analyzed in this paper (see Sect. 3.4). b Taken from Lanza et al. (2009) [L09], Alonso et al. (2008) [A08], Bouchy et al. (2008) [B08], or Czesla et al. (2009) [C09]. c $P_{\rm p}$ - orbital period, $T_{\rm c}$ - central time of first transit, i - orbital inclination, $R_{\rm p}, R_{\rm s}$ - planetary and stellar radii, a - semi major axis of planetary orbit, ua, ub - linear and quadratic limb darkening coefficients.

Source LaTeX | All tables | In the text

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