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Table A.3.
S-G04 component.
| Line | λcenter | z | v | F | FWHM | FWHM |
|---|---|---|---|---|---|---|
| [Å] | [km s−1] | [Å] | [km s−1] | |||
| [N II] λ6583 | 6739.8±0.2 | 0.02376±0.00003 | 7126.5±9. | 1927.±67. | 13.93±0.49 | 620.0±22. |
| Hαλ6563 | 6719.8±0.1 | 0.02392±0.00002 | 7176.8±5. | 1699.±51. | 12.94±0.42 | 577.7±17. |
| [N II] λ6548 | 6704.8±0.4 | 0.02390±0.00010 | 7169.8±31. | 739.4±26. | 13.93±0.49 | 623.3±22. |
| [O I] λ6300 | 6449.1 ±0.3 | 0.02362±0.00004 | 7085.2±14. | 300.2±12. | 14.36±0.57 | 668.0±27. |
| [O III] λ5007 | 5126.0±0.5 | 0.02380±0.00010 | 7139.8±30. | 88.0 ±5. | 9.81±0.44 | 574.1±26. |
| Hβλ4861 | 4979.0:±1.0 | 0.02420±0.00021 | 7261.0±62. | 23.3: ±5. | 8.45:±1.8 | 509.:±107. |
Notes. The table lists: emission line centers, redshifts, line flux F in units of 10−15 erg s−1 cm−2, and line widths (FWHM) of the strongest emission lines.
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