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Table 2

Models discussed in this work.

Model Description
A The base low-resolution model, in which the deep atmosphere is isothermally initialised
B Like model A, but with the deep atmosphere adiabatically initialised
C Mid-resolution version of model A (d = 30)
D High-resolution version of model A (d = 40)
E →I Highly evolved versions of model A, which have reached a deep adiabat and then had deep isothermal Newtonian cooling introduced at various strengths: For E log(τ220) = 7.5, F log(τ220) = 11, G log(τ220) = 15, H log(τ220) = 20, and I log(τ220) = 22.5
J & K Highly evolved versions of model A which have reached a deep adiabat, and then had their outer atmospheric Newtonian cooling modified to reflect a different surface temperature: 1200 K in model J and 2200 K in model K

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