Table 1.
Properties of the sample.
| Field | ID | RA | Dec | z | AGN | log M* | SFR | log Lbol | log L2 − 10 keV | log NH |
|---|---|---|---|---|---|---|---|---|---|---|
| [deg] | [deg] | type | [log M⊙] | [M⊙ yr−1] | [erg s−1] | [erg s−1] | [cm−2] | |||
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) | (11) |
| XMM-XXL | X_N_81_44 | 34.378942 | –4.306572 | 2.311 | BL | 10.89 ± 0.25 | 173 ± 92 | 46.80 ± 0.03 | 44.77 |
< 21.86 |
| CDF-S | XID36 | 52.961556 | –27.784281 | 2.259 | NL | 10.72 ± 0.08 | 186 ± 9 | 45.70 ± 0.06 | 43.84 |
> 24.10 |
| CDF-S | XID419 | 53.097649 | –27.715270 | 2.145 | NL | 10.89 ± 0.02 | 44 ± 2 | 45.54 ± 0.05 | 43.84 |
24.28 |
| COSMOS | cid_1057 | 149.812485 | 2.111014 | 2.214 | NL | 10.99 ± 0.08 | 64 ± 7 | 45.91 ± 0.06 | 44.53 |
23.98 |
| COSMOS | cid_346 | 149.930878 | 2.118734 | 2.219 | BL | 10.67 ± 0.37 | 380 ± 29 | 46.66 ± 0.02 | 44.47 |
23.05 |
| COSMOS | cid_451 | 150.002533 | 2.258629 | 2.450 | NL | 11.21 ± 0.05 | 48 ± 19 | 46.44 ± 0.07 | 45.18 |
23.87 |
| COSMOS | cid_1205 | 150.010696 | 2.332968 | 2.255 | BL (a) | 11.16 ± 0.22 | 88 ± 16 | 45.75 ± 0.17 | 44.25 |
23.50 |
| COSMOS | cid_1143 | 150.036819 | 2.257776 | 2.492 | NL | 10.82 ± 0.04 | 8 ± 2 | 44.85 ± 0.12 | 44.83 |
24.01 |
Notes. All quantities are taken from Circosta et al. (2018), except for the SFRs and stellar masses which have been derived from the SED fitting including the Band 7 fluxes presented in this paper (see Sect. 3.4). (1) Field where the targets are located. (2) Source identification number from the catalogues corresponding to each field. (3) RA and (4) Dec of the optical counterpart. (5) Spectroscopic redshift. (6) AGN classification as broad line (BL) or narrow line (NL) objects according to the optical spectra. (7) Host galaxy stellar mass and 1σ error. (8) SFR from the 8−1000 μm FIR luminosity and 1σ error. (9) AGN bolometric luminosity and 1σ error, derived from SED fitting. (10) Absorption-corrected X-ray luminosity in the hard band (2−10 keV) and 90% confidence level error. (11) Absorbing hydrogen column density and 90% confidence level error, derived from either X-ray spectral fitting or hardness-ratio (see Circosta et al. 2018).
cid_1205 was previously reported as a NL target in Circosta et al. (2018), but it is now classified as a BL target based on the presence of BLR emission in the Hα line in the K-band SINFONI spectrum (Kakkad et al. 2020).
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