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Table 4

Summary of the inputs to the model spectra.

Component Self-consistent Free-chemistry
Temperature
Profile
T.1) mean profile measured by JWST NIRISS/SOSS for orbital phases in Table 5 (see also Fig. A.1) T.2) As T.1) but isothermal above 10−5 bar Isothermal: T=1800 K
Chemistry Ch.1) Equilibrium chemistry for metallicities 0.1, 1, 10, 100, 1000 times solar
Ch.2) Same as Ch.1) but with TiO removed
Ch.3) Same as Ch.1) but with TiO and VO removed
Hydrogen-helium atmosphere with a uniform volume mixing ratio of a single species, log10(VMRx):
x → TiO: {–5,–6,–7,...,–15}
x → VO: {–5,–6,–7,...,–15}
x → Fe: {–2,–3,–4,...,–7}
x → MgH: {–4,–5,–6,...,–14}
x → FeH: {–5,–6,–7,...,–13}
x → H2O: {–1,–2,–3,...,–8}
x → AlH: {–5,–6,–7,...,–13}
Grey cloud deck with an optical depth of 10 spanning one order of magnitude in pressure.
Clouds Mg2SiO4 and MgSiO3 clouds modelled with virga assuming kzz = 109, fsed = 1 and the above temperature profiles Top of the cloud deck pressure, Ptop: 10{0.5,0,-0.5,...,-5} bar
Cloud scattering properties:
Parameter Pre-eclipse (C.1) Post-eclipse (C.2)
ω0 0.885 0.995
g0 0.0 0.0

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