Table 1.
Characteristics of the cosmological simulations used in this work.
| L | mDM | m⋆ | ΩΛ, 0 | Ωm, 0 | Ωb, 0 | σ8 | nS | h | Host | |
|---|---|---|---|---|---|---|---|---|---|---|
| [Mpc] | [M⊙] | [M⊙] | number | |||||||
| COCO | 25 | 1.92 × 105 | 0.728 | 0.272 | 0.04455 | 0.81 | 0.967 | 0.704 | 108 | |
| TNG50 | 50 | 4.5 × 105 | 8.5 × 104 | 0.6911 | 0.3089 | 0.0486 | 0.8159 | 0.9667 | 0.6774 | 60 |
| AURIGA | 148 | 3 × 105 | 5 × 104 | 0.693 | 0.307 | 0.048 | 0.811 | 0.965 | 0.6777 | 30 |
Notes. Column 2 indicates the simulated volume size; for TNG50 and Auriga, L is the length of the 3D cube side; for COCO, L is the radius of the high-resolution region. Columns 3 and 4 indicate the dark matter particle resolution and the stellar mass particle resolution. Since COCO is a collisionless N-body simulation, only a single particle species is used in the high-resolution region, the mass of which (given in the column mDM) includes the contribution of both dark matter and baryons to the total matter density. The particle-tagging treatment of stellar mass in COCO is described in the text. Columns 5–10 indicate the cosmology parameters applied in the simulations. For COCO, the value of Ωb, 0 is that assumed when generating initial conditions in the semi-analytic model. The last column indicates the number of host galaxies used from each of the simulations.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.