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Fig. 10


Expected amplitude of the occultation of the planet as a function of the wavelength for two extreme values for the heat redistribution factor for CoRoT-13b (as defined by Cowan & Agol 2010; ϵ = 1: uniform heat distribution over the planet; ϵ = 0 no distribution) and two values of the Bond albedo. The gray shaded area is the wavelength window observed by CoRoT. The black arrow is the upper limit of CoRoT observations.

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