Fig. 2: JWST G395H spectrum for W1935 overlaid with the best-fitting models with and without temperature inversion. | Nature

Fig. 2: JWST G395H spectrum for W1935 overlaid with the best-fitting models with and without temperature inversion.

From: Methane emission from a cool brown dwarf

Fig. 2: JWST G395H spectrum for W1935 overlaid with the best-fitting models with and without temperature inversion.

Overlaid in purple and dark cyan are the median retrieval models for the source with and without temperature inversion, respectively. Data uncertainties are shaded in grey. The 67% confidence intervals in the model posteriors are shaded in dark cyan and purple but are of comparable extent to the width of the plotted data.

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