Table 4.
Properties of the CIVλ1549 emission line derived from parametric model fits (see Sect. 3.2).
| ID |  |
FWHMCIV | EWCIV |  |
Log (LCIV/erg s−1) | Log (L1350/erg s−1) |
|---|---|---|---|---|---|---|
| (Å) | (km s−1) | (Å) | (km s−1) | |||
| X_N_160_22 | 1548 ± 1 | 3180 ± 280 | 38 ± 1 | 250 ± 70 | 45.03 ± 0.09 | 46.71 ± 0.10 |
| X_N_81_44 | 1546 ± 1 | 6790 ± 250 | 49 ± 2 | 700 ± 110 | 44.77 ± 0.09 | 46.27 ± 0.10 |
| X_N_53_3 | 1547 ± 1 | 4910 ± 480 | 60 ± 2 | 470 ± 140 | 44.67 ± 0.09 | 46.09 ± 0.10 |
| X_N_66_23 | 1548 ± 1 | 2350 ± 210 | 63 ± 2 | 240 ± 30 | 44.35 ± 0.09 | 45.80 ± 0.10 |
| X_N_35_20 | 1545 ± 3 | 5550 ± 1240 | 33 ± 7 | 950 ± 520 | 43.56 ± 0.13 | 45.32 ± 0.10 |
| X_N_12_26 | 1545 ± 1 | 3860 ± 520 | 30 ± 1 | 920 ± 140 | 44.49 ± 0.09 | 46.27 ± 0.10 |
| X_N_4_48 | 1549 ± 1 | 5250 ± 620 | 34 ± 2 | 50 ± 140 | 44.41 ± 0.09 | 46.13 ± 0.10 |
| X_N_102_35 | 1548 ± 1 | 3250 ± 100 | 53 ± 1 | 190 ± 70 | 45.14 ± 0.09 | 46.68 ± 0.10 |
| X_N_115_23 | 1549 ± 1 | 2280 ± 220 | 61 ± 2 | 140 ± 70 | 44.79 ± 0.09 | 46.34 ± 0.10 |
| cid_166 | 1545 ± 1 | 3940 ± 173 | 50 ± 1 | 850 ± 70 | 45.24 ± 0.09 | 46.79 ± 0.10 |
| cid_1605 | 1550 ± 1 | 6090 ± 300 | 70 ± 3 | −120 ± 130 | 44.30 ± 0.09 | 45.76 ± 0.10 |
| cid_346 | 1538 ± 1 | 7470 ± 190 | 30 ± 1 | 2230 ± 80 | 44.66 ± 0.09 | 46.49 ± 0.10 |
| cid_1205 | 1551 ± 1 | 1340 ± 140 | 60 ± 6 | 250 ± 60 | 42.34 ± 0.10 | 43.72 ± 0.11 |
| cid_467 | 1548 ± 1 | 3450 ± 310 | 60 ± 2 | 280 ± 70 | 44.91 ± 0.09 | 46.51 ± 0.10 |
| J1333+1649 | 1538 ± 1 | 5250 ± 170 | 19 ± 1 | 2300 ± 30 | 45.65 ± 0.09 | 47.61 ± 0.10 |
| J1441+0454 | 1525 ± 1 | 9690 ± 200 | 24 ± 1 | 4690 ± 30 | 45.47 ± 0.09 | 47.33 ± 0.10 |
| J1549+1245 | 1553 ± 1 | 5180 ± 120 | 18 ± 1 | −760 ± 50 | 45.10 ± 0.09 | 47.01 ± 0.10 |
| S82X1905 | 1544 ± 1 | 7250 ± 230 | 45 ± 1 | 1070 ± 100 | 44.63 ± 0.09 | 46.24 ± 0.10 |
| S82X1940 | 1547 ± 1 | 6690 ± 260 | 80 ± 3 | 430 ± 110 | 44.41 ± 0.09 | 45.83 ± 0.10 |
| S82X2058 | 1546 ± 1 | 4080 ± 280 | 28 ± 1 | 740 ± 140 | 44.61 ± 0.09 | 46.44 ± 0.10 |
Notes. Columns give the following information for the BLR component of the CIV emission line: (1) target identification, (2) centroid (Å), (3) FWHM (km s−1), (4) rest-frame EW (Å), (5) velocity of the CIV at 50% of the cumulative line flux, (6) logarithm of the extinction-corrected CIV luminosity, and (7) logarithm of the extinction-corrected luminosity at 1350 Å derived from the best-fit values of the power-law model representing the AGN continuum (see Sect. 3).
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