Into the storm: diving into the winds of the ultra-hot Jupiter WASP-76 b with HARPS and ESPRESSO

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Fig. A.13

Posterior distribution of isothermal line retrieval with an added cos θ dependent day- to nightside wind in the lower atmosphere and a vertical wind in the upper atmosphere. The change in the layers was set at p = 10⁻³ bar, with the surface pressure at P₀ = 10 bar.

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