Fig. 6
Comparison of the 1–5 μm spectral-energy distribution of GJ 758 B to the best fitting synthetic spectra from the BT-SETTL14, Morley+12, Saumon+12, and Exo-REM grids. The asterisks represent the expected fluxes in each bandpass from the atmospheric models. The Exo-REM and Exo-REM – NC models completely overlap because, at this combination of Teff and log g, the cloud condensation occurs below the considered pressure grid, effectively making both models cloud-free.
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