Table 2.
Merger and detection rates per year calculated for the LISA mission.
| Model | Detected | Total | w/2 MBHs | Version |
|---|---|---|---|---|
| Croton16 | ||||
| B3H9-n1 | 55.5 | 84.32 | 62.3% | |
| B4H10-n1 | 17.25 | 26.42 | 17.5% | η = 0.1 |
| B5H11-n1 | 7.0 | 11.73 | 7.8% | |
| B3H9-n2 | 62 | 84.37 | 62.3% | |
| B4H10-n2 | 22.5 | 26.44 | 18.3% | η = 0.4 |
| B5H11-n2 | 11.25 | 11.73 | 7.8% | |
| Bower06 | ||||
| B3H9-f1 | 68.5 | 84.17 | 62.2% | |
| B4H10-f1 | 31 | 40.01 | 22.5% | fedd = 0.01 |
| B5H11-f1 | 15.25 | 30.37 | 14.5% | |
| B3H9-f2 | 64.95 | 84.16 | 62.2% | |
| B4H10-f2 | 31 | 40.01 | 22.5% | fedd = 0.001 |
| B5H11-f2 | 22 | 30.36 | 14.5% | |
Notes. In case of Croton16, the n1 and n2 refer to models with η set to 0.1 or 0.4, respectively. For Bower06, f1 and f2 correspond to fedd = 0.01 and fedd = 0.001, respectively. The fourth column shows the percentage of mergers of galaxies both containing central MBHs with respect to all mergers.
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