Table 3.
Results of the Gaussian line fitting performed on the spectra.
| XID | Bv0 | v0 | FWHM |
|---|---|---|---|
| [mJy beam−1] | [km s−1] | [km s−1] | |
| 42 | 0.76 ± 0.05 | 498 ± 14 | 368 ± 32 |
| 539 | 0.47 ± 0.06 | −56 ± 33 | 308 ± 77 |
| 666Blue | 0.46 ± 0.02 | −194 ± 26 | 474 ± 67 |
| 666Red | 0.39 ± 0.03 | 187 ± 12 | 162 ± 27 |
Notes. Columns from left to right: source ID, brightness of the Gaussian peak, central velocity (with respect to the rest-frame at the given redshift) and FWHM. For XID 666 we report the two Gaussian components, simultaneously fit on the whole source region. The blue-shifted and red-shifted components (with respect to the rest-frame velocity) are named 666Blue and 666Red, respectively.
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