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Table 1

Simulation parameters.

Name Σg ν H/r Mc [ME] Lacc [erg/s] κ [cm2/g] rsmooth N orb Resol.

RADL27k0.01 1.25 × 10-3 10-5 0.03 5 1027 0.01 0.125 30,15,4 low, mid, high
RADL0k0.01 1.25 × 10-3 10-5 0.03 5 0.01 0.125 30,15,4 low, mid, high
RADL27k1 1.3 × 10-3 10-5 0.05 5 1027 1 0.125 30,8,4 low, mid, high
RADL0k1 1.3 × 10-3 10-5 0.05 5 1 0.125 30,8,4 low, mid, high
RADL27k1M15 1.3 × 10-3 10-5 0.05 15 1027 1 0.125 30,16,4 low, mid, high
RADL0k1M15 1.3 × 10-3 10-5 0.05 15 1 0.125 30,16,4 low, mid, high
RADL027k0.01LONG 1.3 × 10-3 10-5 0.03 5 1027 0.01 0.25 30,50 low, mid
RADL0k0.01LONG 1.3 × 10-3 10-5 0.03 5 0.01 0.25 30,50 low, mid
ISO 6.8 × 10-4 10-6 0.03 5 0.1 25 mid

Notes. Col. 1 lists each simulation. The following columns give the gas surface density Σp at the position of the planet in units of , viscosity ν in units of , the aspect ratio H/r at the position of the planet, the core mass Mc in Earth mass, the accretion luminosity Lacc in erg/s, the opacity κ in cm2/g, and the smoothing length rsmooth as fraction of the Hill radius. The second-to-last column gives the number of orbits at the position of the planet that were performed at the corresponding resolution level listed in the last column (see Sect. 2.4 for a detailed description of the nonuniform grid used).

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