Table 1
Simulation runs used in this paper.
| Label | mP ∕mJup | mP ∕m⊕ |  |
Opacities (a) |
|---|---|---|---|---|
| CPD occurrence | ||||
| m1 | 0.06 | 20 | 0.1 | 1.0/0.01 |
| m2 | 0.2 | 60 | 0.1 | 0.01 |
| m3 | 0.3 | 90 | 0.1 | 1.0/0.01 |
| m4 | 0.4 | 120 | 0.1 | 1.0/0.01 |
| m5 | 0.75 | 240 | 0.1 | 1.0/0.01 |
| Main simulations | ||||
| C1 (“nominal”) | 1 | 360 | 0.1 | 0.01 |
| H1 (“high opacity”) | 1 | 360 | 0.1 | 1.0 |
| H2 (“deep”) | 1 | 360 | 0.025 | 0.01 |
| C2 (“Bell & Lin”) | 1 | 360 | 0.1 | 0.01 |
Notes. The relation of the runs with the science questions posed in this work is explained in Sect. 1 and parameters are explained in Sect. 2. (a) Opacities used: numbers denote constant opacities κ for all simulations in cm2 g−1, except for simulation C2, which uses Bell & Lin opacities reduced by the factor in the table. All simulation runs have an unperturbed CSD surface density of Σ0 = 100 g cm−2 at the position of the planet. Simulation letters refer to the purpose or expected simulation outcome: m = “mass survey”, C = “cold”, H = “hot”.
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