Optical constants of exoplanet haze analogs from 0.3 to 30 µm: Comparative sensitivity between spectrophotometry and ellipsometry

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Fig. 11

MIR extinction coefficient of the reduced haze analog determined with spectroscopy on the MgF₂ and intrinsic Si samples, and with Mueller ellipsometry on the doped Si sample. The different modes used for the ellipsometric Lorentz model are listed in Table 2. Gaussian and Lorentzian damping are considered to assess the impact on the interband k values.

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