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Table 4.
Mass gap edges (in solar masses) for each metallicity.
| Z | MGap, low | MGap, high | MGap, high(interp) |
|---|---|---|---|
| 10−11 | 99.5 | 239.5 | 232.3 |
| 10−6 | 84.4 | 229.4 | 229.3 |
| 10−4 | 97.1 | 225.5 | 221.6 |
| 0.001 | 76.5 | 186.2 | 185.4 |
| 0.002 | 53.1 | 147.9 | 147.3 |
| 0.004 | 47.3 | 138.2 | 134.2 |
| 0.006 | 45.6 | 131.0 | 129.4 |
| 0.008 | 46.5 | 132.0 | 129.7 |
| 0.01 | 47.4 | 141.1 | 129.9 |
| 0.014 | 47.4 | – | – |
| 0.017 | 47.1 | – | – |
| 0.02 | 34.3 | – | – |
| 0.03 | – | – | – |
Notes. Column 1: Initial metallicity. Column 2: Most massive remnant below the PI mass gap. Column 3: MRemnant defining the upper limit of the mass gap. Column 4: Interpolated smallest BH mass after the PI gap.
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