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Theoretical Transmission Spectra of Exoplanet Atmospheres with Hydrocarbon Haze: Effect of Creation, Growth, and Settling of Haze Particles. II. Dependence on UV Irradiation Intensity, Metallicity, C/O Ratio, Eddy Diffusion Coefficient, and Temperature
2019 The Astrophysical Journal 877 109.
Caption: Figure 23.
Transmission spectrum models for the atmosphere with haze for three different values of the monomer radius, 1 nm (green line, same as the green line in Figure 5), 10 nm (light-blue line), and 20 nm (purple line). The transmission spectrum for the atmosphere without haze is also plotted (black line; same as the black line in Figure 5). As in Figure 5, the horizontal dotted lines represent the transit depths corresponding to pressure levels from 1 × 10−6 bar to 1 bar. Note that the transmission spectrum models are smoothed for clarity.
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