Table 3.
Best solutions per Z bin.
| Cont. | Z | logΦ(H) | log Ptot | Vturb |  |
|---|---|---|---|---|---|
| [Z⊙] | [cm−2 s−1] | [cm−3 K] | [km s−1] | ||
| (1) | (2) | (3) | (4) | (5) | (6) |
| 50–50 | 1 | 18.25 | 14 | 10 | 5.24 |
| 50–50 | 2 | 18 | 14 | 10 | 7.07 |
| 50–50 | 5 | 18.5 | 14 | 10 | 6.35 |
| 50–50 | 10 | 18.75 | 14 | 20 | 5.82 |
| 50–50 | 20 | 19.25 | 14 | 40 | 3.81 |
| 50–50 | 50 | 19.5 | 14 | 40 | 3.31 |
| 20–80 | 1 | 18.5 | 14 | 30 | 4.35 |
| 20–80 | 2 | 18.25 | 14 | 10 | 5.43 |
| 20–80 | 5 | 18.5 | 14 | 20 | 5.36 |
| 20–80 | 10 | 19 | 14 | 40 | 3.98 |
| 20–80 | 20 | 19.75 | 15.5 | 100 | 1.98 |
| 20–80 | 50 | 20 | 16.25 | 100 | 1.55 |
Notes. (1) Percentage contribution from illuminated and dark sides of the cloud, respectively. (2) Metallicity bin of the cloud associated with the minimum χ2 solution. (3) Logarithm of the ionizing flux associated with the minimum χ2 solution. (4) Logarithm of the total pressure of the cloud associated with the minimum χ2 solution. (5) Microturbulent velocity of the cloud associated with the minimum χ2 solution. (6) Minimum χ2 associated with the best fitting solution for each metallicity bin.
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