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Table 6

Broad-line region gas velocities, central black-hole masses and apparent Eddington ratios for 29 broad-line AGNs.

Object v BLR M BH L 15 − 150  keV L15−150/LEdd
(km s-1) (107M) ×1043 erg s-1

PBC J0050.8+7648 3800 7.6 43 0.04
PBC J0149.3−5017 4975 12 1.7 0.001
PBC J0157.3+4715 2600 3.2 4.8 0.01
PBC J0311.9+5029 4370 9.4 5.9 0.005
PBC J0429.7−6703 3840 7.1 4.6 0.005
PBC J0440.8+2739 3300 5.3 2.8 0.004
PBC J0532.7+1346 2000 1.9 1.1 <0.005
PBC J0535.6+4011 1600 1.2 0.7 0.004
PBC J0543.9−4325 1000 0.5 2.2 0.4
PBC J0609.4−6243 2900 4.1 31 0.06
PBC J0635.0−7441 3800 7.6 15 0.02
PBC J0654.5+0703 1700 1.5 0.9 0.005
PBC J0749.2−8634 5500 15 14 0.008
PBC J0803.4+0840 860 0.4 4.3 0.09
PBC J0818.5−1420 9400 43 21 0.004
PBC J0942.1+2342 4000 7.7 0.8 ~0.001
PBC J1002.3+0304 750 0.3 0.9 0.02
PBC J1020.5−0235 11900 69 5.7 ~0.001
PBC J1254.8−2655 4460 9.7 10 0.008
PBC J1349.0+4443 14500 10 9.1 0.007
PBC J1416.8−1158 12400 58 32 0.004
PBC J1540.3+1415-3 4500 9.9 35 0.03
PBC J1846.0+5607 2800 3.6 11 0.02
PBC J2035.2+2604 1600 1.2 7.4 0.05
PBC J2116.2+2519 11700 69 28 0.003
PBC J2123.9+3407 2500 3 17 0.05
PBC J2157.4−0611 3000 6.2 52 0.07
PBC J2248.8+1725 1000 0.5 15 0.2
PBC J2307.9+4015 5300 14 12 0.007

Notes. The final uncertainties on the black hole mass estimates are about 50% of their values. The velocities were determined using Hβ emission line, whereas the apparent Eddington ratios were computed using the 15–150 keV luminosities.

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