Table 1.
Astrophysical populations.
| Name | IC | MZAMS, 1 | q | P | e | SFRD | 𝒩 |
|---|---|---|---|---|---|---|---|
| Pop. III fiducial | LOG1 | Eq. (1) | Eq. (4) | Eq. (5) | Eq. (6) | H22 | 6916 |
| Pop. III optimistic | LAR1 | Eq. (2) | Eq. (4) | Eq. (5) | Eq. (6) | J19 | 119399 |
| Pop. III pessimistic | TOP5 | Eq. (3) | Eq. (7) | Eq. (8) | Eq. (9) | SW20 | 202 |
| Pop. I-II | Fiducial | Eq. (10) | Eq. (4) | Eq. (5) | Eq. (6) | MF17 | 887364 |
Notes. For each model, we list the name of the initial condition configuration (IC), the distribution of the ZAMS masses of the primary star MZAMS, 1, the distribution of the mass ratios q, the distribution of the orbital periods P, the distribution of the orbital eccentricities e, and the adopted SFRD model. The rightmost column reports the total number of mergers from Eq. (16) assuming Tobs = 10 yr.
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