Table A.3.
Extinction-corrected fluxes and restframe equivalent widths of the emission lines in SDSS spectra
| Galaxy | |||||||||
|---|---|---|---|---|---|---|---|---|---|
| J0232+0025 | J0256+0122 | J0815+2942 | J0837+4512 | ||||||
| Line | λ | Ia | EWb | Ia | EWb | Ia | EWb | Ia | EWb |
| Mg II | 2796 | 29.6±6.0 | 14 | 25.5±5.0 | 6 | 39.2±15. | 22 | 12.2±7.1 | 10 |
| Mg II | 2803 | 18.1±5.5 | 8 | 21.9±4.8 | 5 | 20.6±14. | 10 | 8.2±7.0 | 6 |
| [O II] | 3727 | 104.7±8.1 | 130 | 169.3±11. | 85 | 248.9±24. | 232 | 144.7±10. | 258 |
| H9 | 3836 | 7.7±4.2 | 13 | ... | ... | ... | ... | 8.0±6.0 | 46 |
| [Ne III] | 3869 | 46.4±5.7 | 68 | 43.2±5.1 | 38 | 24.1±12. | 21 | 45.8±6.7 | 104 |
| H8+He I | 3889 | 20.0±4.7 | 31 | 20.0±3.9 | 16 | 25.1±12. | 22 | 18.1±6.4 | 48 |
| H7+[Ne III] | 3969 | 30.5±5.0 | 50 | 29.6±4.4 | 26 | 24.2±12. | 27 | 30.8±6.7 | 52 |
| Hδ | 4101 | 31.2±5.0 | 53 | 31.9±4.2 | 30 | 26.2±12. | 24 | 25.1±6.2 | 58 |
| Hγ | 4340 | 48.2±5.5 | 95 | 48.6±5.2 | 47 | 49.1±12. | 56 | 47.6±6.4 | 141 |
| [O III] | 4363 | 7.1±3.8 | 14 | 7.0±3.1 | 5 | 3.8±1.0 | 5 | 8.7±4.9 | 23 |
| Hβ | 4861 | 100.0±6.9 | 281 | 100.0±7.1 | 156 | 100.0±13. | 193 | 100.0±7.3 | 368 |
| [O III] | 4959 | 200.7±9.8 | 610 | 156.9±9.1 | 250 | 159.6±15. | 157 | 177.9±9.2 | 634 |
| [O III] | 5007 | 609.9±20. | 1329 | 452.0±17. | 450 | 502.6±29. | 548 | 514.3±18. | 967 |
| C(Hβ)c | 0.000±0.090 | 0.000±0.092 | 0.000±0.167 | 0.084±0.093 | |||||
| EW(abs)d | 0.0 | 0.0 | 0.0 | 1.0 | |||||
| F(Hβ)e | 7.4±0.3 | 6.0±0.6 | 3.5±0.2 | 8.1±0.3 | |||||
| J0901+5111 | J0908+4626 | J0955+3935 | J1021+0436 | ||||||
| Line | λ | Ia | EWb | Ia | EWb | Ia | EWb | Ia | EWb |
| Mg II | 2796 | 18.2±4.7 | 25 | 19.6±3.8 | 14 | 24.7±4.5 | 14 | 18.2±6.6 | 9 |
| Mg II | 2803 | 11.9±4.4 | 14 | 14.7±3.5 | 8 | 17.9±4.0 | 10 | 14.9±6.5 | 8 |
| [O II] | 3727 | 113.4±8.1 | 253 | 111.7±7.9 | 103 | 176.5±11. | 120 | 126.2±8.6 | 160 |
| H9 | 3836 | 6.2±3.5 | 14 | ... | ... | ... | ... | ... | ... |
| [Ne III] | 3869 | 45.7±5.3 | 79 | 38.0±4.0 | 47 | 35.3±4.8 | 31 | 41.0±6.7 | 62 |
| H8+He I | 3889 | 19.4±4.1 | 64 | 19.7±12. | 17 | 17.9±12. | 9 | 15.8±5.2 | 24 |
| H7+[Ne III] | 3969 | 32.9±4.7 | 80 | 25.7±16. | 25 | 24.6±11. | 27 | 26.9±5.4 | 41 |
| Hδ | 4101 | 27.2±4.4 | 73 | 24.5±12. | 23 | 24.2±9.1 | 20 | 30.5±5.3 | 53 |
| Hγ | 4340 | 48.7±5.1 | 142 | 34.6±14. | 26 | 41.8±8.5 | 42 | 45.6±5.5 | 77 |
| [O III] | 4363 | 13.4±3.5 | 59 | 3.9±2.5 | 3 | 9.6±3.5 | 6 | 4.3±3.0 | 9 |
| Hβ | 4861 | 100.0±6.8 | 281 | 100.0±12. | 112 | 100.0±8.6 | 160 | 100.0±6.5 | 206 |
| [O III] | 4959 | 250.8±11. | 730 | 142.3±8.0 | 208 | 161.3±10. | 217 | 204.9±9.0 | 350 |
| [O III] | 5007 | 722.4±16. | 891 | 425.7±16. | 1045 | 464.7±18. | 435 | 636.3±19. | 907 |
| C(Hβ)c | 0.000±0.088 | 0.050±0.084 | 0.000±0.093 | 0.065±0.084 | |||||
| EW(abs)d | 0.0 | 3.0 | 3.6 | 0.5 | |||||
| F(Hβ)e | 7.4±0.3 | 7.4±0.6 | 6.0±0.6 | 10.5±0.3 | |||||
| J1252+5237 | J1358+4611 | J1450+3913 | |||||||
| Line | λ | Ia | EWb | Ia | EWb | Ia | EWb | ||
| Mg II | 2796 | 39.9±6.8 | 14 | 29.7±4.2 | 10 | 10.0±2.2 | 13 | ||
| Mg II | 2803 | 30.4±6.2 | 11 | 18.7±3.6 | 6 | 9.4±2.3 | 15 | ||
| [O II] | 3727 | 133.8±9.8 | 95 | 165.6±8.9 | 100 | 133.7±7.5 | 106 | ||
| H9 | 3836 | 8.7±3.5 | 8 | 12.2±12. | 7 | 9.7±6.1 | 7 | ||
| [Ne III] | 3869 | 45.4±5.7 | 32 | 36.3±3.9 | 28 | 29.5±3.5 | 24 | ||
| H8+He I | 3889 | 14.4±4.0 | 11 | 19.6±15. | 11 | 17.3±7.4 | 36 | ||
| H7+[Ne III] | 3969 | 27.4±4.7 | 23 | 31.3±13. | 27 | 27.0±6.9 | 21 | ||
| Hδ | 4101 | 27.4±4.7 | 26 | 31.4±11. | 31 | 25.2±6.5 | 11 | ||
| Hγ | 4340 | 47.4±5.2 | 67 | 45.7±13. | 40 | 47.2±7.1 | 41 | ||
| [O III] | 4363 | 8.9±3.1 | 11 | 5.9±2.1 | 6 | 5.7±2.0 | 7 | ||
| Hβ | 4861 | 100.0±6.9 | 137 | 100.0±10. | 154 | 100.0±6.9 | 135 | ||
| [O III] | 4959 | 178.9±9.4 | 203 | 163.8±7.4 | 215 | 157.8±7.4 | 231 | ||
| [O III] | 5007 | 571.2±20. | 1151 | 469.9±13. | 475 | 463.7±15. | 548 | ||
| C(Hβ)c | 0.236±0.090 | 0.136±0.071 | 0.000±0.073 | ||||||
| EW(abs)d | 0.0 | 3.2 | 2.6 | ||||||
| F(Hβ)e | 6.5±0.6 | 10.4±0.7 | 9.8±0.7 | ||||||
Notes. aI = 100×I(λ)/I(Hβ): I(λ) and I(Hβ) are extinction-corrected fluxes of emission lines. bIn angstrom. cExtinction coefficient. dEquivalent width of hydrogen absorption lines in angstrom. eExtinction-corrected flux, but not corrected for fesc(LyC) in 10−16 erg s−1 cm−2.
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