Table A.1.
Comparative between later theoretical studies of AGN in dwarf galaxies using hydrodynamic simulations and this work.
| Reference | Code | Lbox | M⋆ [M⊙] | Lowest | MBH [M⊙]† | BH seeding | Accretion | Positioning |
|---|---|---|---|---|---|---|---|---|
| (Suite) | redshift | [M⊙] | Mode | |||||
| Volume-limited simulations | ||||||||
| I | RAMSES | 10 cMpc | 106-1012 | 2 | 102-1010.5 | 0.24×M⋆ | Bondi | Dynamical |
| (SuperChunk) | Friction | |||||||
| II | GADGET-3 | 2 h−1cMpc | 103-108 | 4 | 102-106.5 | 102-104 | Bondi | Re-positioned |
| III | CHANGA | 25 Mpc | 108-1010 | 0.05 | 106-107.5 | 106 | Bondi | Dynamical |
| (ROMULUS25) | Friction | |||||||
| IV | AREPO | 40 h−1cMpc | 109-1010.5 | 0 | 105-108 | 105 | Bondi | Re-positioned |
| (FABLE) | ||||||||
| V | GIZMO | ≥100 cMpc | 109-1010.5 | 0 | 104-108 | 104-106 | Bondi | Re-positioned |
| (SIMBA) | ||||||||
| RAMSES | ||||||||
| (Horizon-AGN) | ||||||||
| GADGET-3 | ||||||||
| (EAGLE) | ||||||||
| AREPO | ||||||||
| (Illustris) | ||||||||
| TNG100, | ||||||||
| TNG300 | ||||||||
| Non-cosmological ICs | ||||||||
| VI | AREPO | 302 kpc | 2.1×109 | 0 | 105.7 | 105 | Bondi, | Re-positioned |
| (FABLE) | Supply | |||||||
| Zoom-in simulations | ||||||||
| VII | RAMSES | 50 h−1Mpc | 109.6-1010.8 | 2 | 105-107 | 103.6,105 | Bondi | Dynamical |
| (SETH) | Friction | |||||||
| VIII | RAMSES-RT | 10 h−1cMpc | 105.5-108.5 | 5.7 | 104-105.5 | 104 | Bondi, | Dynamical |
| Forced | Friction | |||||||
| IX | CHANGA | 104.5-108.5 | 0 | - | 104-107 | Bondi | Dynamical | |
| (MARVEL-ous Dwarfs, | 25 Mpc | Friction | ||||||
| DC Justice League) | 50 Mpc | |||||||
| X | AREPO | 10 h−1cMpc | 106-108 | 0 | 103-105 | 102-104 | Bondi, | Re-positioned |
| (FABLE) | Supply | |||||||
| This work | AREPO | 67.77 h−1cMpc | 108.4-109.8 | 0 | 105.5-107.1 | 105 | Bondi | Re-positioned |
| (AURIGA) | ||||||||
Notes. Each column represents (1) Work reference; (2) hydrodynamic code (& suite) used in the analysis; (3) box size of the suite; (4) stellar mass range at the lowest redshift; (5) the lowest redshift studied; (6) BH mass range covered at the lowest redshift; (7) BH mass seeding; (8) accretion mode used in the code; (9) method used for BH positioning. (I) Habouzit et al. (2017), (II) Barai & de Gouveia Dal Pino (2019), (III) Sharma et al. (2020), (IV) Koudmani et al. (2021), (V) Haidar et al. (2022), (VI) Koudmani et al. (2019), (VII) Dubois et al. (2015), (VIII) Trebitsch et al. (2018), (IX) Bellovary et al. (2019), (X) Koudmani et al. (2022)
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.