Table 5.
Properties of MgIIλ2800 emission line derived from parametric model fits (see Sect. 3.2).
| ID |  |
FWHMMgII | EWMgII |  |
Log (LMgII/erg s−1) | Log (L3000/erg s−1) |
|---|---|---|---|---|---|---|
| (Å) | (km s−1) | (Å) | (km s−1) | |||
| X_N_160_22 | 2804 ± 1 | 3620 ± 180 | 25 ± 1 | −390 ± 80 | 44.45 ± 0.07 | 46.46 ± 0.06 |
| X_N_81_44 | 2801 ± 1 | 3910 ± 250 | 36 ± 2 | −90 ± 100 | 44.37 ± 0.07 | 46.25 ± 0.06 |
| X_N_53_3 | 2795 ± 1 | 2880 ± 290 | 17 ± 2 | 530 ± 120 | 44.18 ± 0.08 | 46.32 ± 0.06 |
| X_N_66_23 | 2795 ± 3 | 3180 ± 880 | 26 ± 8 | 510 ± 340 | 43.70 ± 0.13 | 45.78 ± 0.07 |
| X_N_4_48 | 2790 ± 4 | 8730 ± 1040 | 83 ± 14 | 1030 ± 380 | 44.27 ± 0.09 | 45.70 ± 0.07 |
| X_N_102_35 | 2800 ± 1 | 4110 ± 190 | 23 ± 1 | −2 ± 80 | 44.33 ± 0.07 | 46.40 ± 0.06 |
| X_N_115_23 | 2803 ± 2 | 4320 ± 550 | 56 ± 8 | −360 ± 210 | 44.12 ± 0.09 | 45.82 ± 0.07 |
| cid_166 | 2803 ± 1 | 5910 ± 340 | 35 ± 2 | −270 ± 140 | 44.64 ± 0.07 | 46.49 ± 0.06 |
| cid_1605 | 2801 ± 1 | 4210 ± 420 | 42 ± 5 | −150 ± 160 | 43.77 ± 0.08 | 45.50 ± 0.07 |
| cid_346 | 2802 ± 2 | 5400 ± 660 | 29 ± 4 | −220 ±250 | 44.03 ± 0.08 | 45.99 ± 0.06 |
| cid_467 | 2801 ± 5 | 5830 ± 1340 | 17 ± 4 | −60 ± 500 | 43.77 ± 0.11 | 45.95 ± 0.06 |
| J1333+1649 | 2794 ± 1 | 3690 ± 80 | 12 ± 0 | 680 ± 30 | 45.15 ± 0.07 | 47.47 ± 0.06 |
| J1441+0454 | 2792 ± 1 | 4010 ± 100 | 20 ± 0 | 880 ± 40 | 44.96 ± 0.07 | 47.05 ± 0.06 |
| J1549+1245 | 2804 ± 1 | 3150 ± 70 | 22 ± 1 | −410 ± 30 | 45.07 ± 0.07 | 47.15 ± 0.06 |
| S82X1905 | 2805 ± 3 | 4430 ± 770 | 20 ± 4 | −530 ± 330 | 43.93 ± 0.10 | 45.98 ± 0.06 |
| S82X1940 | 2788 ± 2 | 3410 ± 500 | 370 ± 271 | 1240 ± 190 | 43.98 ± 0.09 | 43.63 ± 0.57 |
| S82X2058 | 2792 ± 3 | 4490 ± 630 | 30 ± 4 | 910 ± 270 | 44.09 ± 0.09 | 46.09 ± 0.06 |
Notes. Columns give the following information for the BLR component of the MgII emission line: (1) target identification, (2) centroid (Å), (3) FWHM (km s−1), (4) rest-frame EW (Å), (5) velocity of the MgII at 50% of the cumulative line flux, (6) logarithm of the extinction-corrected MgII luminosity, and (7) logarithm of the extinction-corrected luminosity at 3000 Å derived from the best-fit values of the power-law model representing the AGN continuum (see Sect. 3).
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.