Table 1
Range of cluster parameters explored in this study.
| Parameter | Source | Min. | Max. | Unit |
|---|---|---|---|---|
| Xa | 𝒰 | −23.1 | 0 | kpc |
| Ya | 𝒰 | −15 | 15 | kpc |
| Za | 0.8 𝒩(0, 0.25) +0.2 𝒰 | −2.5 | 2.5 | kpc |
| VR | 0.8 𝒩(0, 35) +0.2 𝒰 | −150 | 150 | km s−1 |
| Vϕ-circ | 0.8 𝒩(0, 25) +0.2 𝒰 | −150 | 150 | km s−1 |
| VZ | 0.8 𝒩(0, 15) +0.2 𝒰 | −100 | 100 | km s−1 |
| M | Power lawsb | 40 | 50 000 | Mθ |
| log t | 𝒰 | 6 | 10 | dex |
| [M/H] | 𝒰 | −1 | 0.5 | dex |
| AV | dust maps | 0 | 20 | mag |
| ∆AV/AV | 𝒰 | 0 | 0.5 | mag |
| Q | ??(0.5, 4) | 0.1 | 10 | − |
| rc | 𝒰 | 0.1 | 8 | pc |
| rJ | gal. potential | − | − | pc |
| rt/rJ | 𝒰 | 0.5 | 2 | − |
Notes. 𝒰 denotes a uniform distribution between the minimum and maximum values. (a, b) denotes a normal distribution truncated between the minimum and maximum values, with the mean, a, and standard deviation, b. For some parameters, a weighted combination of both distributions was used. (a)Samples with a total heliocentric distance d > 15 kpc or d < 0.5 kpc were discarded. (b)Samples from a broken power law that favoured low-mass clusters and is flat at high masses; that is, one with slopes (in mass order) of –1.013, –2.606, and 0.0, with break points at 813 M⊙ and 3364 M⊙.
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