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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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