Table 1.
Simulated BHs that are examined in detail throughout this paper.
| BH id | BH mass | z | Figures | Comments |
|---|---|---|---|---|
| 166 | 1.4 × 108 M⊙ | 5, 6 | BH-mergers | |
| 455 | 6.9 × 107 M⊙ | A.1 | BH-mergers | |
| 1049 | 1.8 × 107 M⊙ | 7, 8, 10 | Anti-aligned spin | |
| 936 | 3.3 × 106 M⊙ | A.1 | Smooth accretion | |
| 549 | 5.8 × 105 M⊙ | 0.18 | 9, A.1 | Anti-aligned spin |
| 132 | 1.5 × 105 M⊙ | A.1 | Off centered BH | |
| 146 | 7.8 × 107 M⊙ | A.2 | < 1% LR DM cont. | |
| 348 | 7.1 × 107 M⊙ | A.2 | < 1% LR DM cont. | |
| 541 | 3.5 × 107 M⊙ | A.2, 10 | < 1% LR DM cont. | |
| G9685 | 4.8 × 106 M⊙ | 0 | 3, 4, 10 | Smooth accretion |
| G648 | 1.6 × 107 M⊙ | 0.26 | A.2 | Smooth accretion |
Notes. The upper part of the table indicates primary BHs extracted from NEWHORIZON at z = 0.18. The first five lines correspond to the most massive BHs of our fiducial sample while BH-549 and BH-132 present specific features namely an anti-aligned BH-galaxy spin configuration and a off-centered BH respectively. The last three lines gathers three other massive primary BHs but with a “contamination” of < 0.1% in mass from lower resolution (LR) DM particles. For these latter, we just show their evolution in Appendix A while they are discarded from any statistical analysis. The lower part of the table is related to the additional two BHs from the GALACTICA zooms, G9685 and G648.
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.