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Fig. 10
Reconstruction of elongated shadows of some exoplanets, using the real TLCs. Panel a: Kepler-45b at KIC 5794240, panel b: Kepler-840b at KIC 11517719, panel c: Kepler-670b at KIC 11414511, and panel d: Kepler-6b at KIC 10874614. The solid curves are the polynomial approximations according to Eq. 10).
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