Open Access
Table 1
Cross-identified galaxy clusters with physical properties from the simulation and their ability to show AQN signatures with and without synchrotron radiation in the background at a transition frequency νT in the low-energy regime.
| Cluster name | Mvir | νT |  (no synchrotron) |
 (with synchrotron) |
|---|---|---|---|---|
| [1014 M⊙] | [GHz] | [%] | [%] | |
| Coma | 18.82 | ✗ | ✗ | ✗ |
| Virgo | 9.91 | 382.45 | 53.2 | 19.22 |
| Perseus | 10.75 | ✗ | ✗ | ✗ |
| Centaurus | 10.18 | 6.5 | 50.97 | 0.46 |
| A119 | 10.21 | 3.26 | 50.33 | 0.35 |
| A539 | 6.34 | 71.42 | 52.43 | 5.76 |
| A1185 | 4.42 | ✗ | ✗ | ✗ |
| A2256 | 3.27 | 223.02 | 53.17 | 26.49 |
| A2877 | 2.22 | 24.29 | 51.87 | 4.69 |
| Norma | 0.79 | ✗ | ✗ | ✗ |
| Fornax | 0.61 | 3842.19 | 54.33 | 53.76 |
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