Table A.1
Retrieved atmospheric parameters and prior probability distributions.
| Parameter | Bayesian Prior | Description | Canonical Model | Without C2 H6 | ||
|---|---|---|---|---|---|---|
| Percentile | HPDI | Percentile | HPDI | |||
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𝒰(−12, −0.3) | Mixing ratio of H2O | ![]() |
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𝒰(−12, −0.3) | Mixing ratio of CH4 | ![]() |
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𝒰(−12, −0.3) | Mixing ratio of NH3 | ![]() |
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| log(XCO) | 𝒰(−12, −0.3) | Mixing ratio of CO | ![]() |
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𝒰(−12, −0.3) | Mixing ratio of CO2 | ![]() |
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| log(XHCN) | 𝒰(−12, −0.3) | Mixing ratio of HCN | ![]() |
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𝒰(−12, −0.3) | Mixing ratio of C2H2 | ![]() |
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𝒰(−12, −0.3) | Mixing ratio of C2H6 | ![]() |
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- | - |
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𝒰(−12, −0.3) | Mixing ratio of CH3OH | ![]() |
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𝒰(−12, −0.3) | Mixing ratio of H2S | ![]() |
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𝒰(−12, −0.3) | Mixing ratio of SO2 | ![]() |
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| log(XDMS) | 𝒰(−12, −0.3) | Mixing ratio of DMS | ![]() |
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𝒰(−12, −0.3) | Mixing ratio of CS2 | ![]() |
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𝒰(−12, −0.3) | Mixing ratio of CH3Cl | ![]() |
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| log(XOCS) | 𝒰(−12, −0.3) | Mixing ratio of OCS | ![]() |
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𝒰(−12, −0.3) | Mixing ratio of N2O | ![]() |
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| T0/K | 𝒰(50, 600) | Temperature at 1 μbar | ![]() |
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- | Temperature at 10 mbar | ![]() |
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𝒰(0.02, 2.00) | P-T profile curvature | ![]() |
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𝒰(0.02, 2.00) | P-T profile curvature | ![]() |
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| log(P1/bar) | 𝒰(−6, 2) | P-T profile region limit | ![]() |
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| log(P2/bar) | 𝒰(−6, 2) | P-T profile region limit | ![]() |
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| log(P3/bar) | 𝒰(−2, 2) | P-T profile region limit | ![]() |
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| log(Pref/bar) | 𝒰(−6, 2) | Reference pressure at RP | ![]() |
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| log(a) | 𝒰(−4, 10) | Rayleigh enhancement | ![]() |
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| γ | 𝒰(−20, 2) | Scattering slope | ![]() |
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| log(Pc/bar) | 𝒰(−6, 2) | Cloud top pressure | ![]() |
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| fc | 𝒰(0, 1) | Cloud and haze fraction | ![]() |
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𝒰(−250, 250) | NIRISS dataset offset | ![]() |
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Note. For the parameter estimates, the central values and uncertainties in the Percentile columns correspond to the median and 16–84% percentiles (1-σ), with values in brackets corresponding to the 2-σ upper limits. The equivalent values in the Highest Posterior Density Interval (HPDI) columns correspond to the mode and HPDI for 68.27% of the probability. The temperature at 10 mbar, which corresponds to the observed photosphere, is derived from the retrieved P − T profile.
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