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Table 3.
BH properties of dust-obscured quasars from different estimators.
| Object name | log(Lbol/erg s−1) |
log(MBH/M⊙) |
||||||
|---|---|---|---|---|---|---|---|---|
| Pβ | Pα | L15(a) | Pβ | Pα | L15 | |||
| F2M0036−0113 | 45.46±0.22 | – | – | 7.85±0.19 | – | – | ||
| F2M0729+3336 | – | – | 46.55 | – | – | 8.70±0.13 (b) | ||
| F2M0817+4354 | – | 45.14±0.23 | – | – | 8.24±0.28 | – | ||
| F2M0830+3759 | – | – | 46.05 | – | – | 8.69±0.11 (b) | ||
| F2M0841+3604 | – | – | 45.95 | – | – | 8.65±0.26 (c) | ||
| F2M1113+1244 | 46.49±0.28 | – | 46.84 | 8.43±0.24 | – | 8.64±0.18 (b) | ||
| F2M1209−0107 | 46.21±0.26 | – | – | 8.87±0.29 | – | – | ||
| F2M1227+5053 | 46.20±0.32 | – | – | 8.52±0.36 | – | – | ||
| F2M1307+2338 | 45.24±0.21 | 45.53±0.25 | – | 7.79±0.20 | 8.06±0.24 | – | ||
| F2M1313+1453 | 46.30±0.25 | – | – | 8.79±0.25 | – | – | ||
| F2M1434+0935 | 46.21±0.25 | – | – | 8.02±0.18 | – | – | ||
| F2M2325−1052 | 46.12±0.37 | – | – | 8.48±0.46 | – | – | ||
Notes.
(a)
The uncertainty for L15 is not provided by Urrutia et al. (2012). The uncertainty for Lbol presented in Fig. 11 was estimated on the assumption that L15’s uncertainty amounts to 10% of its value.
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