Table A.2.
Target sample properties summary, for both AGN and host galaxies.
ID | AGN type |
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SFR (M⊙ yr−1) |
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X-ray net counts |
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---|---|---|---|---|---|---|---|---|---|---|
(1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) | (11) |
X_N_160_22 | BL | – | – | – | 46.74 ± 0.02 | 24.5 ± 4.9 | < 22.32 |
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8.9 ± 0.2 | < 24.87 |
X_N_81_44 | BL | 11.04 ± 0.37 | 45.93 ± 0.20 | 229 ± 103 | 46.80 ± 0.03 | 94.8 ± 9.7 | < 21.86 |
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9.2 ± 0.1 | < 24.81 |
X_N_53_3 | BL | – | 46.41 ± 0.11 | 686 ± 178 | 46.21 ± 0.03 | 25.8 ± 5.1 |
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8.7 ± 0.1 | < 24.86 |
X_N_66_23 | BL | 10.96 ± 0.29 | < 46.00 | < 268 | 46.04 ± 0.02 | 118.7 ± 10.9 | < 21.51 |
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8.3 ± 0.2 | < 24.84 |
X_N_35_20 | BL | – | – | – | 45.44 ± 0.02 | 38.1 ± 6.2 | < 22.27 |
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8.7 ± 0.1 | < 24.79 |
X_N_12_26 | BL | – | – | – | 46.52 ± 0.02 | 61.3 ± 7.8 | < 20.90 |
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8.9 ± 0.1 | < 24.88 |
X_N_44_64 | BL | 11.09 ± 0.25 | 45.93 ± 0.15 | 229 ± 80 | 45.51 ± 0.07 | 51.8 ± 7.2 | < 21.97 |
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9.1 ± 0.2 | < 24.78 |
X_N_4_48 | BL | – | – | – | 46.16 ± 0.02 | 58.2 ± 7.6 | < 21.85 |
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9.1 ± 0.2 | < 24.81 |
X_N_102_35a | BL | – | – | – | 46.82 ± 0.02 | 79.0 ± 8.9 | < 22.17 |
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8.9 ± 0.1 | 27.05 ± 0.01 |
X_N_115_23 | BL | – | – | – | 46.49 ± 0.02 | 131.8 ± 11.5 | < 22.26 |
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8.4 ± 0.1 | < 24.82 |
XID36a | NL | 10.68 ± 0.07 | 45.84 ± 0.02 | 184 ± 9 | 45.70 ± 0.06 | 47.2 ± 6.9 | b> 24.1 |
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– | 25.40 ± 0.01 |
XID57 | NL | 10.49 ± 0.11 | < 45.10 | < 34 | 44.26 ± 0.18 | 58.9 ± 7.7 |
b
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– | < 24.20 |
XID419 | NL | 10.89 ± 0.02 | 45.20 ± 0.04 | 42 ± 4 | 45.54 ± 0.05 | 70.2 ± 8.4 |
b
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– | < 24.12 |
XID427 | NL | 10.87 ± 0.08 | < 45.43 | < 72 | 44.60 ± 0.13 | 324.2 ± 18.0 |
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– | < 24.20 |
XID522 | NL | 10.42 ± 0.02 | 46.26 ± 0.02 | 492 ± 25 | 45.02 ± 0.02 | 35.1 ± 5.9 | b> 22.5 |
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– | 24.37 ± 0.05 |
XID614 | NL | 10.78 ± 0.08 | 45.97 ± 0.02 | 247 ± 12 | 44.97 ± 0.13 | 78.3 ± 8.8 |
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– | < 24.26 |
cid_166 | BL | 10.38 ± 0.22 | < 45.92 | < 224 | 46.93 ± 0.02 | 717.8 ± 26.8 | < 21.25 |
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9.3 ± 0.1c | < 24.00 |
lid_1289 | NL | 9.59 ± 0.14 | < 44.98 | < 25 | 45.09 ± 0.08 | 123.4 ± 11.1 |
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– | < 23.98 |
cid_1057 | NL | 10.84 ± 0.07 | 45.50 ± 0.02 | 85 ± 4 | 45.91 ± 0.06 | 36.1 ± 6.0 |
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– | < 23.89 |
cid_1605 | BL | – | < 45.54 | < 94 | 46.03 ± 0.02 | 327.9 ± 18.1 |
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8.4 ± 0.2 | < 23.84 |
cid_337 | NL | 11.13 ± 0.04 | 45.63 ± 0.03 | 115 ± 9 | 45.34 ± 0.09 | 83.1 ± 9.1 | < 22.76 |
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– | 23.99 ± 0.07 |
cid_346a | BL | 11.01 ± 0.22 | 46.13 ± 0.06 | 362 ± 49 | 46.66 ± 0.02 | 124.1 ± 11.1 |
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8.9 ± 0.1c | 24.86 ± 0.07d |
cid_451a | NL | 11.21 ± 0.05 | < 45.67 | < 125 | 46.44 ± 0.07 | 136.9 ± 11.7 |
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– | 26.43 ± 0.01d |
cid_1205 | NL | 11.20 ± 0.10 | 46.16 ± 0.04 | 384 ± 33 | 45.75 ± 0.17 | 33.9 ± 5.8 |
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– | 24.10 ± 0.06 |
cid_2682 | NL | 11.03 ± 0.04 | < 45.54 | < 93 | 45.48 ± 0.10 | 35.5 ± 6.0 |
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– | < 23.99 |
cid_1143a | NL | 10.40 ± 0.17 | 45.61 ± 0.07 | 108 ± 18 | 44.85 ± 0.12 | 51.3 ± 7.2 |
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– | 24.39 ± 0.05 |
cid_467 | BL | 10.10 ± 0.29 | < 45.74 | < 147 | 46.53 ± 0.04 | 446.8 ± 21.1 |
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8.9 ± 0.6 | < 23.92 |
cid_852 | NL | 11.17 ± 0.02 | < 45.57 | < 100 | 45.50 ± 0.11 | 25.0 ± 5.0 |
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– | < 23.90 |
cid_971 | NL | 10.60 ± 0.12 | – | < 96e | 44.71 ± 0.24 | 33.1 ± 5.8 | < 23.68 |
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– | < 24.01 |
Notes. (1) Target ID, see also Table A.1; (2) AGN classification into broad line (BL) and narrow line (NL) according to the optical spectra; (3) Galaxy stellar mass and 1σ error; (4) FIR luminosity in the 8 − 1000 μm range and 1σ error; (5) SFR from the FIR luminosity and 1σ error; (6) AGN bolometric luminosity and 1σ error, derived from SED fitting; (7) X-ray net counts (i.e., background subtracted) in the full band and respective error, computed assuming a Poisson statistic; (8) Absorbing hydrogen column density and 90% confidence level error; (9) Absorption-corrected X-ray luminosity in the hard band (2 − 10 keV) and 90% confidence level error; (10) Black hole mass and 1σ error. For the XMM-XXL and Stripe82X targets the values are from Shen et al. (2015), for the WISSH targets are from Weedman et al. (2012), and for COSMOS we have re-analyzed zCOSMOS and FMOS spectra (Schulze et al., in prep.); (11) Radio power at 1.4 GHz and 1σ error.
Targets classified as “jetted” (Padovani 2017), according to the comparison between their IR and radio properties (see Fig. 7).
Targets fit with the physical model MYtorus (Murphy & Yaqoob 2009) that self-consistently takes into account photoelectric absorption, Compton scattering, cold reflection and fluorescent emission in a fixed toroidal geometry. The analysis was performed as described in Lanzuisi et al. (2018).
BH mass derived using the Hβ emission line from Subaru/FMOS spectroscopy (Schulze et al., in prep.).
Targets detected at 1.4 GHz as part of the VLA-COSMOS survey (Schinnerer et al. 2007). The luminosities reported here for these targets are derived from the 1.4 GHz fluxes. The predicted 3 GHz fluxes (assuming αr = 0.7) are consistent with the observed 1.4 GHz ones for cid_1253 and cid_346, while for cid_451 the predicted flux is a factor of 2 higher than the measured 1.4 GHz one. The measurements reported for the other COSMOS targets are derived from 3 GHz fluxes (see Sect. 4.3).
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