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Table 1.

Model grids used as input for MCMC exploration.

Model Teff
(K)
ΔT
(K)
log g
log10
(cgs)
Δlog g
log10
(cgs)
(M/H)
(dex)
Δ(M/H)
(dex)
fsed Δfsed Remarks
BT-Settl 1200–3000 100 3.0–5.5 0.5 0.0
petitCODE(0) 500–1700 50 3.0–6.0 0.5 −1.0 to 1.4 0.2 Cloud-free
petitCODE(1) 1000–1500 100 2.0–5.0 1.0 −1.0 to 1.0 1.0 1.5 w/o scattering, w/o Fe clouds
petitCODE(2) 1000–1500 100 2.0–5.0 0.5 0.0–1.5 0.5 0.5–6.0 1.0a with scattering, w/o Fe clouds
petitCODE(3) 1000–2000 200 3.5–5.0 0.5 −0.3 to 0.3 0.3 1.5 With scattering, with Fe clouds
Exo-REM(1) 400–2000 100 3.0–5.0 0.1 0.32, 1.0, 3.32 Cloud particle size fixed to 20 μm
Exo-REM(2) 400–2000 100 3.0–5.0 0.1 0.32, 1.0, 3.32 1.0

Notes. The radius of the planet was included as an additional analytic fit-parameter regardless of the model, ranging from 0.1 RJ to 5 RJ.

(a)

Except additional grid point at 0.5.

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