Table 2.
Global properties and measurements of the strengths of stellar He IIλ1640 emission, N Vλ1240, and C IVλ1550 absorption.
| Name | MUV | SFR |
 |
12 + log(O/H) | EW0 (N V) | EW0 (C IV) | EW0 (He II) | FWHM (He II) |
|---|---|---|---|---|---|---|---|---|
| (AB) | (M⊙ yr−1) | (log [M⊙]) | (Å) | (Å) | (Å) | (km s−1) | ||
| J0006+2452 | −24.17 | 316 ± 31 | 9.50 ± 0.05 | 8.49 ± 0.10 | −3.78 ± 0.40 | −6.70 ± 0.19 | 4.54 ± 0.38 | 2070 ± 180 |
| J0031+3545 | −24.62 | 390 ± 60 | 9.59 ± 0.07 | – | −2.11 ± 0.48 | −5.40 ± 0.34 | 2.29 ± 0.58 | 1800 ± 430 |
| J0036+2725 | −23.91 | 612 ± 62 | 9.79 ± 0.05 | – | −5.40 ± 0.34 | −6.29 ± 0.19 | 2.69 ± 0.35 | 2810 ± 470 |
| J0110−0501 | −23.33 | 110 ± 15 | 9.04 ± 0.06 | 8.48 ± 0.15 | −4.87 ± 0.64 | −4.32 ± 0.35 | 4.57 ± 0.59 | 1990 ± 510 |
| J0115+1837 | −23.52 | 210 ± 35 | 9.33 ± 0.07 | 8.37 ± 0.12 | −2.08 ± 0.76 | −4.22 ± 0.29 | 3.80 ± 0.47 | 2870 ± 165 |
| J0121+0025 | −24.11 | 460 ± 90 | 9.65 ± 0.08 | – | −3.54 ± 0.20 | −5.51 ± 0.20 | 3.06 ± 0.33 | 3170 ± 580 |
| J0146−0220 | −23.68 | 340 ± 43 | 9.53 ± 0.06 | 8.47 ± 0.20 | −3.38 ± 0.46 | −3.87 ± 0.27 | 2.99 ± 0.42 | 2480 ± 135 |
| J0850+1549 | −23.76 | 190 ± 26 | 9.28 ± 0.06 | 8.27 ± 0.13 | −1.18 ± 0.46 | −2.27 ± 0.31 | 1.37 ± 0.44 | 2030 ± 1351 |
| J1013+4650 | −23.67 | 210 ± 27 | 9.32 ± 0.05 | 8.45 ± 0.10 | −2.64 ± 0.53 | −6.16 ± 0.27 | 3.45 ± 0.46 | 2520 ± 310 |
| J1157+0113 | −23.40 | 195 ± 68 | 9.29 ± 0.13 | – | −2.32 ± 1.12 | −2.41 ± 0.62 | 3.02 ± 0.92 | 2280 ± 260 |
| J1220+0842 | −24.36 | 360 ± 32 | 9.56 ± 0.04 | 8.13 ± 0.19 | −3.16 ± 0.29 | −2.00 ± 0.21 | 2.52 ± 0.33 | 1150 ± 20 |
| J1316+2614 | −24.65 | 415 ± 115 | 9.62 ± 0.11 | 8.45 ± 0.12 | −1.87 ± 0.68 | −3.82 ± 0.54 | 4.48 ± 0.14 | 2370 ± 85 |
| J1335+4330 | −23.64 | 920 ± 150 | 9.96 ± 0.08 | 8.33 ± 0.17 | −2.70 ± 0.88 | −3.64 ± 0.34 | 3.40 ± 0.51 | 2350 ± 200 |
Notes. The He IIλ1640 emission EW0 is measured by integrating normalized flux in the spectral regions from 1630 Å to 1655 Å. The N Vλ1240 and C IVλ1550 absorption EW0 are measured by integrating normalized flux in the spectral regions from 1230 Å to 1240 Å, and 1530 Å to 1543 Å respectively.
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