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Fig. 13
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Refractive indices n (top) and k (middle and bottom) from UV to FIR of hydrocarbon exoplanet haze analogs produced without nitrogen with the PAMPRE and COSmIC setups. Data for the Exoplanet 2 and Exoplanet 3 analogs produced from different gas relative abundances CH4/CO (see Table 1) are shown.
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