Revisiting the conundrum of the sub-Jovian and Neptune desert - A new approach that incorporates stellar properties

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Table 2

Bayesian evidence for the models defined in this work.

Model	ln ℰ (upper boundary)	ln ℰ (lower boundary)
$ℳ_{1}^{R}$ ${\cal M}_1^R$	6.4655	–6.7525
$ℳ_{2}^{R}$ ${\cal M}_2^R$	–16.6151	–44.4909
$ℳ_{3}^{R}$ ${\cal M}_3^R$	–25.7549	–69.6771
$ℳ_{1}^{M}$ ${\cal M}_1^M$	–3.4143	–4.4521
$ℳ_{2}^{M}$ ${\cal M}_2^M$	–26.0992	–15.7327

Notes. The models favoured in the model comparison process is highlighted with a grey band.

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