Fig. 2
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Transmission spectra obtained on the Titan 1 and Exoplanet 2 PAMPRE haze analogs (see Table 1) from 0.3 to 2.5 μm. Top: data and analysis using the Swanepoel method for the Titan 1 sample produced from a gas mixture of 90% N2 and 10% CH4. Bottom: data and best fit using Cauchy and Tauc–Lorentz dispersion laws for the Exoplanet 2 analog produced from 95% Ar and 5% CH4 in the initial gas mixture.
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