Table 2.
Properties of the eight simulated systems classified as major mergers and the two galaxies that are not involved in any major mergers.
| System ID | z | rm [kpc] | μC | μ⋆ | Log(M⋆/M⊙) | Log(SFR/M⊙ yr−1) |
|---|---|---|---|---|---|---|
| Major merging galaxies | ||||||
| H2 | 4.495 | 11.3 | 2.0 | 4.1 | 10.44 | 1.84 |
| H4 | 4.495 | 16.3 | 2.3 | 1.5 | 10.55 | 1.96 |
| H5 | 4.495 | 6.3 | 1.3 | 1.9 | 10.49 | 1.83 |
| H6 | 4.495 | 5.3 | 1.3 | 1.9 | 10.43 | 1.81 |
| H10 | 4.495 | 10.3 | 3.2 | 1.3 | 10.51 | 1.90 |
| H25 | 4.495 | 40.3 | 2.8 | 2.3 | 10.30 | 1.70 |
| H28 | 4.495 | 32.3 | 3.6 | 4.1 | 10.27 | 1.74 |
| H0 | 4.988 | 13.3 | 4.6 | 1.5 | 10.58 | 2.17 |
| Non-interacting galaxies | ||||||
| H7 | 4.495 | – | – | – | 10.43 | 1.84 |
| H29 | 4.495 | – | – | – | 10.58 | 1.85 |
Notes. For each redshift, z, we show the system ID, the distance obtained averaging over distances between merging galaxies on the x, y, z projections, rm [kpc], the carbon mass ratio, μC, the relative mass ratio of the merging pair, μ⋆, the total stellar mass, M⋆ and SFR. In the last two rows, we report integrated properties for non-interacting systems which we use together with merging systems; see the discussion in Sect. 5.
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