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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.
- Provider: AAS Journals
Caption: Figure 5.
Transmission spectrum models for the atmosphere with haze (green line) and without haze (black line) for the fiducial case. 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 with the resolution R of 100.
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