Open Access
Table A.2
Film thicknesses determined for each COSmIC haze analog from the reflection spectra obtained in the UV-Visible-NIR spectral range.
| COSmIC analog | Gas composition | Spectral range | Position a | Film thickness (nm) |
|---|---|---|---|---|
| Titan 1 | 90% N2–10% CH4 | 0.4-1.67 μm | 1 | 1134.0 |
| 2 | 1031.1 | |||
| 3 | 990.1 | |||
| 4 | 1108.9 | |||
| Titan 2 | 95% N2−5% CH4 | 0.4-1.67 μm | 1 | 798.2 |
| 2 | 1023.0 | |||
| 3 | 802.6 | |||
| Pluto | 95% N2−4.95% CH4−0.05% CO | 0.4-1.67 μm | 1 | 762.4 |
| 2 | 624.5 | |||
| 3 | 574.8 | |||
| 4 | 875.0 | |||
| Exoplanet 1 | 95% N2–4% CH4–1% CO | 0.35-1.65 μm | 1 | 813.8 |
| 2 | 688.5 | |||
| 3 | 722.7 | |||
| 4 | 809.2 | |||
| Exoplanet 2 | 95% Ar–5% CH4 | 0.35-1.67 μm | 1 | 447.8 |
| 2 | 464.6 | |||
| Exoplanet 3 | 95% Ar–4% CH4−1% CO | 0.3-1.67 μm | 1 | 611.2 |
| 2 | 647.0 | |||
| 3 | 559.0 | |||
| 4 | 611.4 | |||
| 5 | 509.8 |
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