Fig. 3
Contributions of the absorbing species to our best-fit transmission spectrum at nominal irradiation within the K2 to Spitzer spectral range. The H2O cloud is not forming in this case, so there is no cloud contribution. The spectral contribution of individual species takes the CIA and Rayleigh scattering (represented as a dotted curve) into account. The spectral contribution of FeH, TiO, and VO are not represented here as they are insignificant.
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