Table 6.
Viewing inclinations, SMBH masses estimates from model (Col. 3), from observations (Col. 4), and from reverberation mapping (Col. 5).
| Object | i(°) | log(MMOD/M⊙) | log(MPOL/M⊙) | log(MREV/M⊙) |
|---|---|---|---|---|
| 25.01 | 7.2 ± 0.2 | |||
| NGC 4051 | 32.46 | 6.92 ± 0.09 | 6.69 ± 0.21 | 6.24 ± 0.13 |
| 38.62 | 6.78 ± 0.06 | |||
| 25.01 | 7.56 ± 0.07 | |||
| NGC 4151 | 32.46 | 7.40 ± 0.03 | 7.21 ± 0.27 | 7.12 ± 0.05 |
| 38.62 | 7.27 ± 0.04 | |||
| 25.01 | 8.94 ± 0.09 | |||
| 3C 273 | 32.46 | 8.90 ± 0.09 | 8.85 ± 0.27 | 8.83 ± 0.11 |
| 38.62 | 8.87 ± 0.08 | |||
| 25.01 | 8.00 ± 0.08 | |||
| PG0844+349 | 32.46 | 7.95 ± 0.06 | 7.70 ± 0.23 | 7.85 ± 0.21 |
| 38.62 | 7.88 ± 0.06 |
Notes. M pol denotes masses obtained using AP15 which we used as input mass. Masses obtained by reverberation mapping were taken from Bentz & Katz (2015) using virial factor 〈f〉 = 4.31 ± 1.05 (Grier et al. 2013).
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