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.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.