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Table 1.
Priors used in the modelling.
| Parameter | Description | Prior |
|---|---|---|
| fin, NSC | In situ NSC mass fraction | (0.0, 1.0) |
| η | Mass fraction in clusters | (10−5, 0.5) |
| Mgal | Host stellar mass | Measured |
| Mcl, min | Least massive GC ever | (10, 100) |
| Mcl, max | Most massive GC ever | (MGC, max, 7.6 × 107) and < ηMgal |
| MGC, lim | Limiting mass for inspiral | ∼MGC, max or model prediction from LvdV21 |
| Mdiss | Dissolution mass limit | ∼MGC, min |
Notes. Masses in M⊙. Except for fin, NSC, the priors are implemented in logarithmic units. Theoretical limit on Mcl, max from Norris et al. (2019a).
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