Fig. 1.
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Conductivity profile of this work (black) in comparison with that of Kumar et al. (2021) for HD 209458 b. The references above the lines indicate the atmosphere model used by Kumar et al. (2021) to compute the respective conductivity profile, namely: Guillot (2010), Line et al. (2016), and Spiegel et al. (2009) with and without TiO in the atmosphere.
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