Planetary eclipse mapping of CoRoT-2a - Evolution, differential rotation, and spot migration

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Table 1:

Stellar/planetary parameters of CoRoT-2a/b.
Star^a	Value $\pm$ Error	Ref.
$P_{\rm s}$	$(4.522 ~ \pm ~ 0.024)$ d	L09
Spectral type	G7V	B08
Planet^b	Value $\pm$ Error	Ref.
$P_{\rm p}$	$(1.7429964 ~ \pm ~ 0.0000017)$ d	A08
$T_{\rm c}$ [BJD]	$(2~454~237.53562 ~ \pm ~ 0.00014)$ d	A08
i	$(87.7 ~ \pm ~ 0.2)$ $^{\circ}$	C09
$R_{\rm p}/R_{\rm s}$	$(0.172 ~ \pm ~ 0.001)$	C09
$a/R_{\rm s}$	$(6.70 ~ \pm ~ 0.03)$	A08
u_a, u_b	$(0.41\pm0.03), (0.06\pm 0.03)$	A08

References. taken from Lanza et al. (2009) [L09], Alonso et al. (2008) [A08], Bouchy et al. (2008) [B08], or Czesla et al. (2009) [C09].

Notes. ^(a) $P_{\rm s}$ - stellar rotation period; ^(b) P_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, u_a, u_b - linear and quadratic limb darkening coefficients.

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