Signature of the atmospheric asymmetries of hot and ultra-hot Jupiters in light curves

Open Access

Fig. 7

Difference between the flux (Eq. (2)) of a 1D solid sphere (batman) and the flux of a 3D simulation of an ultra-hot Jupiter (Pytmosph3R) without rotation (i.e., N_𝒯 = 1). The ultra-hot Jupiter is WASP-121b (Fig. 4). The x axis shows the wavelength; the y axis shows the transit phase.

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