Table 1
Parameters of the simulations performed.
| Interpolation models | ζ/ζ0 | Aυ (mag) | T (K) | M/Φ ((M/Φ)0) |  |
|---|---|---|---|---|---|
| Fiducial | 1 | 10 | 10 | 0.5 | 300 |
| Low ζ | 0.5 | 10 | 10 | 0.5 | 300 |
| High ζ | 2 | 10 | 10 | 0.5 | 300 |
| Medium Aυ | 1 | 5 | 10 | 0.5 | 300 |
| Low Aυ | 1 | 3 | 10 | 0.5 | 300 |
| Low T | 1 | 10 | 6 | 0.5 | 180 |
| High T | 1 | 10 | 15 | 0.5 | 450 |
High  |
1 | 10 | 10 | 0.5 | 750 |
| Generalized models | ζ/ζ0 | Aυ (mag) | T (K) | M/Φ ((M/Φ)0) |  |
|---|---|---|---|---|---|
| Random ICs | 1.48 | 8.9 | 11.4 | 0.29 | 526 |
| Medium T | 1 | 10 | 8 | 0.5 | 300 |
High  ,T |
1 | 10 | 12.5 | 0.5 | 400 |
| Low M/Φ | 1 | 10 | 10 | 0.25 | 300 |
| High M/Φ | 1 | 10 | 10 | 0.75 | 300 |
| Supercritical | 1 | 10 | 10 | 2.6 | 300 |
| High Aυ | 1 | 20 | 10 | 0.5 | 300 |
Notes. Top: simulations used in the interpolation function to calculate the resistivities. Bottom: simulations tested blindly. From left to right columns we list the name of the simulation, the cosmic-ray ionization rate, the visual extinction, the temperature, the mass-to-flux ratio, and the initial density. Here, ζ0 = 1.3 × 10−17 s−1 is the standard value of the cosmic-ray ionization rate (Caselli et al. 1998) and the mass-to-flux ratio is given in units of the critical value (Mouschovias & Spitzer 1976).
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