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Table 1.
Best-fitting parameters (top row of each entry) and weighted standard deviations σ (bottom row) derived through the radiative transfer model RT-scat applied to the down-the-barrel stacked spectra in bins of stellar mass and SFR, assuming the gas as a smooth medium.
| Smooth | logNMgII | vexp | vran | vemit | EWint |
|---|---|---|---|---|---|
| Medium | [cm−2] | [km/s] | [km/s] | [km/s] | [Å] |
| 14.5 | 150 | 25 | 25 | 4.0 | |
| All | 0.2 | 39 | 6 | 4 | 0.5 |
| 14.5 | 100 | 50 | 25 | 3 | |
| High mass | 0.7 | 27 | 11 | 59 | 2 |
| 13.5 | 400 | 25 | 25 | 3.0 | |
| Low mass | 0.03 | 41 | 37 | 8 | 0.1 |
| 14.5 | 150 | 25 | 50 | 2 | |
| High SFR | 0.9 | 25 | 8 | 33 | 2 |
| 13.5 | 500 | 50 | 25 | 2.00 | |
| Low SFR | 0.0 | 21 | 43 | 7 | 0.01 |
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