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Fig. 3

image

Examples of reconstruction of the thermal profile of the transit chord for the case of an unspotted stellar disk. The orbital parameters used in the simulation are listed in Table 1. From top to bottom, we show the case of (i) a stellar disk with no LD, noise-free LC and λ = 0; (ii) a stellar disk with LD, noise-free LC and λ = 0; (iii) a stellar disk with LD and LC with a photometric precision of 1 mmag and λ = 23; (iv) a stellar disk with LD and LC with a photometric precision of 0.1 mmag and λ = 2.9.

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