Table 3.
Predicted number of quasar counterparts and their i-band luminosities for black holes in the literature for which masses and Eddington ratio estimates exist, assuming the system to be in a binary.
| Name | MBH (108 M⊙) | z | ηEdd | dNgw, QSO/dlog10MBH | mi |
|---|---|---|---|---|---|
| J0005−0006 | 0.8 | 5.844 | 5.5 | 6160.0 | 26.0 |
| J0028+0457 | 28.8 | 5.99 | 0.29 | 41140.0 | 19.0 |
| J0033−0125 | 26.3 | 6.02 | 0.1 | 54110.0 | 18.0 |
| J0050+3445 | 25.7 | 6.253 | 0.55 | 31810.0 | 20.0 |
| J0055+0146 | 2.4 | 5.983 | 1.07 | 197070.0 | 23.0 |
| J0100+2802 | 107.2 | 6.3 | 1.2 | 60.0 | 20.0 |
| J0109−3047 | 13.5 | 6.763 | 0.3 | 118070.0 | 21.0 |
| J0136+0226 | 3.1 | 6.21 | 0.55 | 875690.0 | 23.0 |
| J0210−0456 | 0.8 | 6.438 | 2.19 | 26050.0 | 26.0 |
| J0221−0802 | 6.9 | 6.161 | 0.3 | 317130.0 | 21.0 |
| J036.5078+03.0498 | 30.2 | 6.533 | 0.54 | 28060.0 | 20.0 |
| J0227−0605 | 1.8 | 6.21 | 0.95 | 638920.0 | 24.0 |
| J0303−0019 | 3.3 | 6.079 | 0.91 | 316340.0 | 23.0 |
| J0305−3150 | 9.1 | 6.61 | 0.68 | 137820.0 | 22.0 |
| J0353+0104 | 15.8 | 6.072 | 0.68 | 57800.0 | 21.0 |
| J0836+0054 | 11.0 | 5.81 | 0.51 | 139390.0 | 21.0 |
| J0841+2905 | 10.0 | 5.95 | 0.87 | 73890.0 | 22.0 |
| J0842+1218 | 19.1 | 6.069 | 0.63 | 50420.0 | 21.0 |
| J1030+0524 | 13.2 | 6.302 | 0.74 | 59000.0 | 21.0 |
| J1048+4637 | 19.1 | 6.198 | 1.17 | 910.0 | 21.0 |
| J167.6415−13.4960 | 3.0 | 6.505 | 1.26 | 13900.0 | 24.0 |
| J1120+0641 | 25.1 | 7.087 | 0.59 | 30270.0 | 21.0 |
| J1137+3549 | 52.5 | 6.01 | 0.33 | 15410.0 | 19.0 |
| J1148+5251 | 50.1 | 6.407 | 0.48 | 13150.0 | 19.0 |
| J1148+0702 | 14.8 | 6.34 | 0.74 | 53860.0 | 21.0 |
| J1205−0000 | 47.9 | 6.73 | 0.06 | 21940.0 | 17.0 |
| J1207+0630 | 44.7 | 6.03 | 0.17 | 22790.0 | 18.0 |
| J1250+3130 | 7.8 | 6.14 | 1.35 | 2880.0 | 23.0 |
| J1306+0356 | 11.0 | 6.017 | 0.87 | 62820.0 | 22.0 |
| J1335+3533 | 40.7 | 5.9 | 0.32 | 24480.0 | 19.0 |
| J1342+0928 | 7.8 | 7.527 | 1.55 | 2510.0 | 23.0 |
| J1411+1217 | 10.7 | 5.903 | 1.32 | 1980.0 | 22.0 |
| J1427+3312 | 7.6 | 6.12 | 1.17 | 3290.0 | 22.0 |
| J1429+5447 | 13.2 | 6.12 | 0.52 | 89510.0 | 21.0 |
| J1509−1749 | 29.5 | 6.121 | 0.62 | 25050.0 | 20.0 |
| J231.6576−20.8335 | 30.9 | 6.587 | 0.5 | 29150.0 | 20.0 |
| J1602+4228 | 15.5 | 6.08 | 0.95 | 26130.0 | 21.0 |
| J1623+3112 | 14.1 | 6.211 | 0.68 | 64020.0 | 21.0 |
| J1630+4012 | 11.0 | 6.058 | 0.68 | 103230.0 | 21.0 |
| J1641+3755 | 2.4 | 6.047 | 2.04 | 9900.0 | 24.0 |
| J2100−1715 | 9.3 | 6.087 | 0.43 | 203290.0 | 21.0 |
| J323.1382+12.2986 | 14.1 | 6.592 | 0.47 | 91730.0 | 21.0 |
| J2229+1457 | 1.2 | 6.152 | 2.14 | 24070.0 | 25.0 |
| J338.2298+29.5089 | 27.5 | 6.66 | 0.12 | 51190.0 | 19.0 |
| J2310+1855 | 43.7 | 5.96 | 0.58 | 14290.0 | 20.0 |
| J2329−0301 | 2.5 | 6.417 | 1.17 | 19120.0 | 24.0 |
| J2348−3054 | 20.4 | 6.902 | 0.18 | 83130.0 | 20.0 |
| J2356+0023 | 38.9 | 6.05 | 0.03 | 35350.0 | 17.0 |
Notes. We use the compilation in Kim & Im (2019), which includes the latest results from UV and FIR surveys of high-redshift quasars.
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