Image Details
Caption: Figure 18.
Comparison of the spectrum derived here for LHS 1140b and those of K2-18 b (Tsiaras et al. 2019) as well as TRAPPIST-1 e and f (de Wit et al. 2018). Overplotted for each is a forward model assuming a clear H/He-dominated atmosphere with a water abundance of ﹩{\mathrm{log}}_{10}({V}_{{{\rm{H}}}_{2}{\rm{O}}})=-3﹩.
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