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Table 6

Fitting solutions corresponding to the comparison of GJ 504b photometry to atmospheric models using the G goodness-of-fit indicator.

BT-SETTL Morley ATMO Exo-REM petitCODE
R constrained (“hot start” models, 19 Myr →5.8 Gyr)
Teff (K) 550 575 550 550 550
log g (dex) 3.5 3.5 4.0 4.9 4.0
[MH] (dex) 0: 0.0 0.5 0.5 0.2
Kzz(cm2 s−1) 106: 108.5
fsed 2.0 3.0
fcloud 1: 1: 0.75 1:
γ 1.3
R(RJup) 0.82 0.85 0.96 0.84 0.94
M(MJup) 0.9 0.9 3.7 22.8 3.6
log (LL) −6.25 −6.14 −6.11 − 6.23 −6.13
G 9.356 1.301 0.820 1.066 0.553

R unconstrained
Teff (K) 750a 625a 600 550 600
log g (dex) 3.5 4.0 3.5 4.9 3.5
[MH] (dex) 0.0: 0.0 0.0 0.5 0.0
Kzz(cm2 s−1) 106: 108.5
fsed 2.0 2.5
fcloud 1: 1: 0.75 1:
γ 1.3
R(RJup) 0.37 0.64 0.79 0.84 0.78
M(MJup) 0.2 1.7 0.8 22.8 0.8
log (LL) −6.40 −6.25 −6.13 −6.23 −6.14
G 1.378 1.165 0.684 1.066 0.543

Notes. The reported masses are derived from the radius and log g. (a)The fitting solutions predict a H3-band flux in disagreement with the upper limit set by the IRDIS observations.

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