Table 2.
Characteristics of the main simulations used throughout the present paper.
| UNIT | PNG-UNIT | LR-UNIT | FASTPM mocks | |
|---|---|---|---|---|
| Code | L-GADGET 2 | L-GADGET 2 | L-GADGET 2 | FASTPM |
| Nparticles | 40963 | 40963 | 20483 | 20483 |
| mp (h−1 M⊙) | 1.24 × 109 | 1.24 × 109 | 9.97 × 109 | 9.97 × 109 |
| fNL | 0 | 100 | 0 and 100 | 0 and 100 |
| Halo finder | ROCKSTAR | ROCKSTAR | ROCKSTAR | FoF |
| Softening length (h−1 kpc) | 6.1 | 6.1 | 12.2 | 244.14* |
Notes. We refer to the simulations as PNG-UNIT/UNIT while we leave the names PNG-UNITSIMS/UNITSIMS for the simulation suites. From top to bottom: the gravity solver, the number of dark matter particles, the particle mass, the values of fNL set in the initial conditions, the halo finder and the softening length. All the simulations have a box size of Lbox = 1 h−1 Gpc. The cosmological parameters and the input power spectrum are the same (except for fNL) between all the simulations.
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