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Table 2
Emission lines best-fit model.
Line component | Observed wavelength | Err. | Redshift | Err. | Velocity offset | Err. | FWHM | Err |
λ [Å]) | z | [km s-1] | [km s-1] | |||||
|
||||||||
[O II] | 7712.7 | 0.9 | 1.0686 | 0.0002 | – | – | 990 | 110 |
[Ne III] | 8001.5 | 2.6 | 1.0683 | 0.0006 | – | – | 1100 | 250 |
|
||||||||
Si III∗ | 2474.1 | 1.5 | 1.0505 | 0.0014 | –2590 | 200 | 1100 | 450 |
Lyα (narrow abs.) | 2514.9 | 0.5 | 1.0695 | 0.0004 | – | – | 500 | 70 |
Lyα (narrow em.) | 2510.9 | 0.5 | 1.0662 | 0.0004 | – | – | 1980 | 170 |
Lyα (broad em.) | 2494.3 | 4.0 | 1.0525 | 0.0041 | –2430 | 480 | 9300 | 500 |
Lyα (broad abs.) | 2475.4 | 2.5 | 1.0368 | 0.0020 | – | – | 7630 | 250 |
N V∗ (broad em.) | 2540.0 | 10.0 | 1.0470 | 0.0081 | –3100 | 1200 | 10 000 | 800 |
N V (broad abs.) | 2528.3 | 5.0 | 1.0376 | 0.0040 | – | – | 3600 | 600 |
|
||||||||
C IV1550 (narrow abs.) | 3208.7 | 0.3 | 1.0689 | 0.0014 | – | – | 300 | 60 |
C IV1548 (narrow abs.) | 3203.2 | 0.3 | 1.0689 | 0.0005 | – | – | 300 | 60 |
C IV (broad em.) | 3180.9 | 4.4 | 1.0529 | 0.0028 | –2300 | 400 | 10 800 | 560 |
C IV (broad abs.) | 3138.6 | 5.0 | 1.0256 | 0.0032 | – | – | 6800 | 760 |
C IV? (narrow em) | 3194.9 | 1.0 | – | – | – | – | 1208 | 360 |
|
||||||||
Al III∗ | 3828.9 | 2.8 | 1.0614 | 0.0015 | –1030 | 220 | 3800 | 150 |
C III] (narrow em.) | 3943.0 | 1.4 | 1.0660 | 0.0005 | – | – | 1300 | 150 |
C III] (broad em.) | 3926.6 | 3.5 | 1.0572 | 0.0018 | –1640 | 270 | 7750 | 350 |
|
||||||||
Mg II (broad em.) | 5748.3 | 6.9 | 1.0536 | 0.0025 | –2160 | 360 | 13 800 | 470 |
Mg II (broad abs.) | 5687.0 | 4.5 | 1.0317 | 0.0016 | – | – | 5510 | 870 |
Mg II? (narrow em.) | 5775.6 | 1.6 | – | – | – | – | 1490 | 330 |
|
||||||||
No broad absorption emission line best fit results | ||||||||
|
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Lyα (broad em.) | 2501.4 | 2.1 | 1.0583 | 0.0010 | –1470 | 250 | 8200 | 250 |
C IV (broad em.) | 3197.2 | 1.2 | 1.0634 | 0.0008 | –739 | 110 | 10 800 | 580 |
Mg II (broad em.) | 5775.0 | 1.7 | 1.0631 | 0.0007 | –780 | 100 | 13 500 | 440 |
Notes. The lines marked with an asterisk are not used to the average velocity offset. Question marks indicate emission lines of uncertain origin.
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