Table 1.
Main properties of our models.
| ID | MIMBH | MGC | ρGC | γGC | a | e | BH | mBH,min/max | Z | Nsim |
|---|---|---|---|---|---|---|---|---|---|---|
| M⊙ | M⊙ | M⊙ | ||||||||
| S0 | 102 − 105 | 1.7 × 104 − 1.7 × 107 | Dehnen | 0.5 | density | thermal | SM17 | 3.3−53.4 | 0.0002 | 1000 × 4 |
| S1 | 102 − 105 | 1.7 × 104 − 1.7 × 107 | Dehnen | 1.0 | density | thermal | SM17 | 3.3−53.4 | 0.0002 | 1000 × 4 |
| S2 | 102 − 105 | 1.7 × 104 − 1.7 × 107 | Plummer | 0.0 | density | thermal | SM17 | 3.3−53.4 | 0.0002 | 1000 × 4 |
| S3 | 102 − 105 | 1.7 × 104 − 1.7 × 107 | Dehnen | 0.5 | density | thermal | O+16 | 3−30 | 0.0002 | 1000 × 4 |
| S4 | 102 − 105 | 1.7 × 104 − 1.7 × 107 | Dehnen | 0.5 | density | thermal | FLAT | 3−30 | 0.0002 | 1000 × 4 |
| S5 | 102 − 105 | 1.7 × 104 − 1.7 × 107 | Dehnen | 0.5 | logflat | thermal | SM17 | 3.3−53.4 | 0.0002 | 1000 × 4 |
| S6 | 102 − 105 | 1.7 × 104 − 1.7 × 107 | Dehnen | 0.5 | density | thermal | SM17 | 2.8 − 25 | 0.02 | 1000 × 4 |
Notes. Column 1: set ID. Column 2: IMBH mass range. Column 3: Cluster mass range. Column 4: adopted cluster density profile. Column 5: inner slope of the cluster density profile. Columns 6 and 7: distribution adopted for the semimajor axis and eccentricity. Column 8: adopted stellar BH mass spectrum. Column 9: stellar BH mass range. Column 10: metallicity of BH progenitors. Column 11: number of simulations performed.
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