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Fig. 9

image

Reconstruction of circular shadows of some exoplanets, using the real TLCs. Panel a: Kepler-1b at KIC 11446443, panel b: Kepler-12b at KIC 11804465, panel c: Kepler-17b at KIC 10619192, and panel d: Kepler-422b at KIC 9631995. The solid curves are the polynomial approximations according to Eq. (10).

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