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Table 3.
Ultraviolet line measurements for individual galaxies with high enough S/N for the lines.
| He IIλ1640 |
O III] λ1661 + λ1666 |
C III] λ1909 |
|||||||
|---|---|---|---|---|---|---|---|---|---|
| ID | Flux | FWHM | EW | Flux | FWHM | EW | Flux | FWHM | EW |
| (erg s−1 cm−2) | (km s−1) | (Å) | (erg s−1 cm−2) | (km s−1) | (Å) | (erg s−1 cm−2) | (km s−1) | (Å) | |
| Narrow | |||||||||
| CDFS015374 | 1.1 | 240 | 1.7 | 1.6 ± 1.4 | 250 ± 150 | 3.2 ± 2.8 | 3.1 ± 2.4 | 510 ± 300 | 6.5 ± 5.0 |
| CDFS023170 | 2.8 | 455 | 1.1 | 1.3 ± 1.1 | 315 ± 300 | 0.7 ± 0.6 | 6.5 ± 2.4 | 850 ± 150 | 3.2 ± 0.4 |
| CDFS023527 | 1.5 | 260 | 0.9 | 2.6 ± 1.4 | 270 ± 110 | 1.6 ± 0.9 | 8.7 ± 3.1 | 580 ± 110 | 6.9 ± 2.4 |
| CDFS113062 | 4.0 | 640 | 1.4 | 2.4 ± 1.8 | 450 ± 225 | 0.9 ± 0.7 | 12.3 ± 2.2 | 630 ± 50 | 5.6 ± 1.0 |
| CDFS126819 | 9.5 | 860 | 8.0 | 2.4 ± 1.8 | 220 ± 170 | 2.4 ± 1.8 | 9.9 ± 4.0 | 820 ± 150 | 8.0 ± 3.2 |
| UDS013586 | 3.1 | 335 | 0.6 | 2.8 ± 2.4 | 400 ±130 | 0.6 ± 0.5 | 12.0 ± 3.1 | 800 ± 100 | 3.3 ± 0.8 |
| UDS019505 | 2.0 | 530 | 0.7 | 2.2 ± 2.0 | 420 ± 140 | 0.9 ± 0.8 | 8.3 ± 2.4 | 860 ± 120 | 4.5 ± 1.3 |
| UDS281893 | 2.9 | 660 | 1.1 | 2.1 ± 1.1 | 450 ± 70 | 0.9 ± 0.5 | 7.1 ± 1.3 | 600 ± 60 | 4.1 ± 0.2 |
| CDFS009705 | 2.2 | 510 | 1.3 | – | – | – | 8.6 ± 1.1 | 820 ± 50 | 6.3 ± 0.8 |
| CDFS229681 | 1.2 | 520 | 1.9 | – | – | – | 3.9 ± 2.7 | 600 ± 290 | 8.6 ± 6.0 |
| Broad | |||||||||
| UDS137388 | 23.1 | 1420 | 4.6 | – | – | – | 16.0 ± 6.3 | 1100 ± 280 | 5.0 ± 2.0 |
Notes. Line fluxes are in units of 10−18 erg s−1 cm−2. The O III] FWHM given in the table is for the λ1666 line. The errors on He II line properties are given in Table 1.
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