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Table 2.

Properties of BLR components of the Hβ emission line derived from parametric model fits.

ID Log (/erg s−1)
(Å) (km s−1) (Å)
X_N_160_22 4876 ± 1 5190 ± 170 58 ± 2 43.99 ± 0.04
X_N_81_44 4873 ± 1 5290 ± 170 57 ± 2 43.87 ± 0.04
X_N_12_26 4865 ± 1 4890 ± 200 51 ± 2 43.58 ± 0.04
X_N_4_48 4860 ± 4 6710 ± 670 40 ± 4 42.95 ± 0.06
X_N_102_35 4872 ± 1 4810 ± 160 58 ± 2 43.67 ± 0.04
X_N_115_23 4869 ± 2 6330 ± 250 56 ± 2 43.68 ± 0.04
cid_166 4867 ± 1 6970 ± 130 91 ± 2 44.17 ± 0.04
cid_1605 4860 ± 3 5040 ± 510 156 ± 22 43.25 ± 0.06
cid_346 4870 ± 2 6280 ± 340 46 ± 2 43.63 ± 0.05
cid_467 4875 ± 5 9260 ± 760 93 ± 8 43.62 ± 0.05
J1333+1649 4841 ± 7 6300 ± 250 42 ± 2 45.34 ± 0.04
J1441+0454 4855 ± 1 4030 ± 100 47 ± 1 44.73 ± 0.04
J1549+1245 4867 ± 2 16570 ± 690 108 ± 7 45.53 ± 0.05
S82X1905 4872 ± 1 4960 ± 100 71 ± 1 43.80 ± 0.04
S82X1940 4862 ± 1 3710 ± 140 75 ± 3 43.24 ± 0.04
S82X2058 4860 ± 1 6450 ± 150 69 ± 1 43.78 ± 0.04

Notes. Columns give the following information for the BLR component of the Hβ emission line: (1) target identification, (2) centroid (Å), (3) FWHM (km s−1), (4) rest-frame EW (Å), (5) logarithm of the extinction-corrected Hβ luminosity.

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