The Hot-Neptune Initiative (HONEI) - I. Two hot sub-Neptunes on a close-in eccentric orbit (TOI-5800 b) and a farther-out circular orbit (TOI-5817 b)

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Table B.5

Prior parameter distribution for the calculation of the internal compositions of TOI-5800 b and TOI-5817 b.

Parameter	Prior range	Distribution
Fe/Si_mantle . . . . . . . .	0–Fe/Si_star	uniform
Mg/Si_mantle . . . . . . . .	Mg/Si_star	Gaussian
M_core/(M_core + M_mantle) . .	0.1–0.9	uniform
H₂-He-H₂O atmosphere
Z . . . . . . . . . . . .	0–1	uniform
L (erg s⁻¹) . . . . . . . .	(2.0–3.1) × 10²¹	log-uniform
M_atm/M_p . . . . . . . .	0.001–0.1	log-uniform
Pure water case
M_{water, bulk}/M_p . . . . . .	0.03–0.5	uniform

Notes. The parameters Z, L, and M_atm are only used in the case of uniformly mixed atmosphere, while the parameter M_{water, bulk}, referring to the bulk water content of a planet, is only used in the pure water case.

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