Table 2
Values of MBH, Lbol, and E(B − V) for red quasars.
| Object name | MBH | Lbol | Eddington ratio |  a |
 b |
 |
 |
 |
|---|---|---|---|---|---|---|---|---|
| (108 M⊙) | (1046 erg s−1) | (mag) | (mag) | (mag) | (mag) | (mag) | ||
| 0036−0113 | 0.60 ± 0.12 | 0.61 ± 0.03 | 0.830 | 0.79 | 0.96 ± 0.10 | >1.58 | 0.98 ± 0.07 | 2.54 ± 0.26d |
| 0817+4354 | – | – | – | 0.73 | – | – | 2.40 ± 0.19 | – |
| 0825+4716 | 12.25 ± 2.98* | 10.40 ± 1.02* | 0.693* | 0.71 | 0.52 ± 0.10 | 1.59 ± 0.27 | – | – |
| 0911+0143 | 2.59 ± 0.44* | 1.54 ± 0.16* | 0.486* | – | 0.63 ± 0.17 | – | – | – |
| 0915+2418 | 10.94 ± 4.92* | 12.95 ± 3.18* | 0.967* | 0.68 | 0.36 ± 0.12 | – | – | – |
| 1113+1244 | 3.09 ± 0.52* | 8.92 ± 0.67* | 2.360* | 1.15 | 1.41 ± 0.11 | 0.45 ± 0.09 | – | – |
| 1209−0107 | 8.75 ± 2.71 | 3.25 ± 0.21 | 0.303 | 0.89 | – | – | – | – |
| 1227+5053 | 2.87 ± 1.00* | 2.26 ± 0.49* | 0.644* | 0.38 | – | 0.23 ± 0.11 | – | –0.23 ± 0.07c |
| 1248+0531 | 2.49 ± 0.32* | 1.93 ± 0.12* | 0.633* | – | 0.26 ± 0.07 | – | – | – |
| 1307+2338 | 0.49 ± 0.11 | 0.32 ± 0.02 | 0.525 | 0.58 | 0.75 ± 0.09 | >1.47 | 1.46 ± 0.08 | 1.74 ± 0.10d |
| 1309+6042 | 2.37 ± 0.26* | 1.80 ± 0.09* | 0.622* | – | 0.95 ± 0.13 | 1.29 ± 0.07 | – | – |
| 1313+1453 | 7.62 ± 0.92* | 4.65 ± 0.17* | 0.499* | – | 1.12 ± 0.15 | – | – | – |
| 1434+0935 | 0.95 ± 0.11* | 3.88 ± 0.13* | 3.350* | – | 1.14 ± 0.10 | 0.81 ± 0.08 | – | – |
| 1532+2415 | 6.12 ± 4.87* | 2.24 ± 1.05* | 0.299* | 0.70 | – | >2.11 | – | – |
| 1540+4923 | 11.86 ± 7.13* | 2.73 ± 1.11* | 0.188* | – | 0.97 ± 0.10 | – | – | – |
| 1600+3522 | 1.81 ± 0.49* | 4.26 ± 0.63* | 1.927* | 0.22 | – | – | – | – |
| 1656+3821 | 4.87 ± 0.98* | 4.66 ± 0.53* | 0.783* | 0.61 | 0.88 ± 0.16 | >0.30 | – | – |
| 1720+6156 | 1.31 ± 0.33* | 2.58 ± 0.38* | 1.613* | – | 1.50 ± 0.09 | 0.57 ± 0.28 | – | – |
| 2325−1052 | 2.71 ± 1.59* | 2.02 ± 0.73* | 0.610* | 0.50 | – | 0.64 ± 0.21 | – | 0.56 ± 0.01d |
| 2339−0912 | 5.95 ± 0.95* | 8.03 ± 0.55* | 1.102* | 1.06 | 1.25 ± 0.06 | 0.53 ± 0.07 | – | – |
Notes. (*) MBH, Lbol values, and Eddington ratios are adopted from Kim et al. (2015b). (a) 
values are adopted from Glikman et al. (2007), which uncertainties are not available. (b) 
values are adopted from Urrutia et al. (2009). (c) 
values are measured with total line luminosities. (d) 
values are measured with broad line luminosities.
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