DREAM - III. A helium survey in exoplanets on the edge of the hot Neptune desert with GIANO-B at TNG

Open Access

Fig. A.1

Light curves (left panels) and the limb-darkening ratio, namely, $\frac{L D_{j}}{L D_{mean}}$ ${{L{D_{\rm{j}}}} \over {L{D_{{\rm{mean}}}}}}$ with j the orbital phase (right panels) computed with the Python batman code (Kreidberg 2015) and the system parameters from Table A.2. The contact points t₁, t₂, t₃, and t₄ are marked with vertical black lines. Blue dots are the light curves and limb-darkening ratio at the observed phases.

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