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Table D.3

BLR gas velocities (in km s-1), central black hole masses (in units of 108M), Eddington luminosity, and apparent Eddington ratios for broad line AGNs discussed in this paper.

Object v BLR M BH L Edd L BOL / L Edd

2PBCJ0057.2+6401 5803 11 136 0.09
2PBCJ0217.07250 10622 25 308 0.04
2PBCJ0440.66507 5046 0.5 6.4 0.10
2PBCJ0550.72304 2550 0.1 0.7 0.44
2PBCJ0653.11227 5184 5 62 0.12
2PBCJ0709.53538 2986 0.2 2.3 0.05
2PBCJ0714.62521 4086 0.2 2.6 0.09
2PBCJ0757.9+0113 9241 2.4 30 0.06
2PBCJ0812.34003 3229 1.8 22 0.03
2PBCJ1228.10925 16600 123 1542 0.01
2PBCJ1251.85127 6732 4.5 57 0.09
2PBCJ1520.20433 2937 1.1 14 0.09
2PBCJ1709.72349 1180 0.1 1.0 0.19
2PBCJ1742.06053 7895 11 138 0.03
2PBCJ2030.77530 4076 2.5 31 0.06
2PBCJ2045.9+8321 2325 0.2 3.1 2.41
2PBCJ2048.3+3812 11448 3.7 46 0.03
2PBCJ2136.3+2003 4501 0.7 8.4 0.07
2PBCJ2155.1+6205 2475 0.1 0.8 0.36
2PBCJ2348.9+4153 2373 0.2 3.1 0.76

2PBC J2010.32522 1575 1.3 16 15.4

Notes. The final uncertainties on the black hole mass estimates are about 50% of their values. The velocities were determined using Hβ emission or Mg ii (upper and lower part of the table, respectively), whereas the apparent Eddington luminosity (in units of 1045 erg s-1) and ratios were computed using the bolometric luminosity obtained from the (observed or rescaled, see text) 15–150 keV luminosities.

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