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Table D.1.

Priors and inferred parameters from the MCMC analysis obtained with HADES codes.

Planetary parameters Prior Final estimate
Mass (Mp/MJup) [0.1, 8.0] 6 . 1 0.9 + 0.7 $ 6.1^{+0.7}_{-0.9} $
Intrinsic Temp. (Tint) [K] [300, 1500] 1000 ± 30
Metallicity ([Fe/H]) [dex] [ − 2, 3] 0 . 1 0.4 + 0.8 $ 0.1^{+0.8}_{-0.4} $
Core Mass (Mcore/M) [1, 100] Unconstrained3
Sedimentation (fsed) [1, 6] 2 . 8 0.8 + 1.1 $ 2.8^{+1.1}_{-0.8} $
Vertical Mixing (log Kzz) [1, 12] 9 . 0 1.5 + 1.2 $ 9.0^{+1.2}_{-1.5} $
Radius (RJup) Model derived 1.4 ± 0.1

Notes. All priors are uniform in the given ranges. The reported values are the median of the marginalized posterior distribution, with errors corresponding to the 16th and 84th percentiles.

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