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Fig. A.5
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MCMC probability distribution of the Gaussian profile parameters for the Ca II IRT λ8500 Å and λ8664 Å (top row), and the He I λ10830 Å (corrected and masked tellurics, bottom row) absorption lines observed in the transmission spectrum of WASP-76b. The distributionswere obtained using 104 steps and 10 walkers.
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