Table 1
Our sample from the COSMOS field.
| Object ID | RA | Dec | z | log(Lbol) | log(mbh) | log(NH) | Macc | L/Ledd | Log M ∗ | SFR |
| (h:m:s) | °:′:′′ | (erg/s) | (M⊙) | (cm-2) | (M⊙/yr) | (M⊙) | (M⊙/yr) | |||
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) | (11) |
|
|
||||||||||
| 178 | 10 00 14 | 02 28 37 | 1.253 | 45.7 | 7.78 | 22.3 | 0.8 | 0.6 | 10.8 | 134 |
| 5330 | 09 59 30 | 02 41 26 | 2.169 | 45.9 | 8.22 | 22.5 | 1.2 | 0.4 | 10.5 | 101 |
| 5627 | 09 58 44 | 01 43 09 | 1.337 | 45.7 | 8.77 | 22.0 | 0.8 | 0.07 | 10.4 | 157 |
| 54204 | 09 58 20 | 02 03 02 | 1.356 | 46.1 | 8.27 | 22.9 | 1.7 | 0.5 | 10.7 | 438 |
| 2028 | 10 02 11 | 01 37 07 | 1.592 | 46.3 | 8.83 | 21.9 | 2.8 | 0.2 | 11.6 | 250 |
Notes. Column (1): the X-ray ID of the objects; Cols. (2) and (3): optical coordinates (J200); Col. (4): the spectroscopic redshift of the targets; Col. (5): bolometric luminosity from SED fitting; Col. (6): black hole mass from broad MgII lines; Col. (7): column density from X-ray spectral fits; Col. (8): mass accretion rate of the black hole; Col. (9): the Eddington ratio of the black hole; Col. (10): stellar mass of the host galaxy and Col. (11): star formation rate of the host galaxy following the procedure by Bonzini et al. (2015). See Sect. 2 for a detailed description of the selection procedure.
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