Table A.1.
Summary of AGN and host galaxy properties for the target sample.
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) |
X_N_128_48 | BL | – | – | – | 45.81 ± 0.40 (a) | 12 ± 4 | < 22.80 |
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10.04 ± 0.3 (b) |
X_N_81_44 | BL | 11.04 ± 0.37 | 45.93 ± 0.20 | 229 ± 103 | 46.80 ± 0.03 | 95 ± 10 | < 21.86 |
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9.05 ± 0.30 (c) |
X_N_53_3 | BL | – | 46.41 ± 0.11 | 686 ± 178 | 46.21 ± 0.03 | 26 ± 5 |
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8.53 ± 0.30 (c) |
X_N_6_27 | BL | – | < 45.90 | < 215 | 45.85 ± 0.05 | 26 ± 5 | < 22.64 |
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8.73 ± 0.30 (d) |
X_N_44_64 | BL | 11.09 ± 0.25 | 45.93 ± 0.15 | 229 ± 80 | 45.51 ± 0.07 | 52 ± 7 | < 21.97 |
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8.76 ± 0.31 (c) |
X_N_102_35 | BL | – | – | – | 46.82 ± 0.02 | 79 ± 9 | < 22.17 |
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8.85 ± 0.30 (c) |
X_N_104_25 | BL | – | – | – | 45.97 ± 0.40 (a) | 80 ± 9 | < 21.91 |
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8.91 ± 0.30 (d) |
lid_1852 | NL | 10.07 ± 0.13 | < 45.28 | < 52 | 45.25 ± 0.09 | 53 ± 7 |
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– |
lid_3456 | BL | 10.75 ± 0.30 | 46.08 ± 0.17 | 323 ± 126 | 45.68 ± 0.07 | 5 ± 2 | < 22.00 |
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7.64 ± 0.33 (d) |
cid_166 | BL | 10.38 ± 0.22 | < 45.92 | < 224 | 46.93 ± 0.02 | 718 ± 27 | < 21.25 |
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9.33 ± 0.30 (c) |
lid_1289 | NL | 9.59 ± 0.14 | < 44.98 | < 25 | 45.09 ± 0.08 | 123 ± 11 |
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– |
cid_1605 | BL | - | < 45.54 | < 94 | 46.03 ± 0.02 | 328 ± 18 |
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8.55 ± 0.31 (c) |
cid_337 | NL | 11.13 ± 0.04 | 45.63 ± 0.03 | 115 ± 9 | 45.34 ± 0.09 | 83 ± 9 | < 22.76 |
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– |
cid_346 | BL | 11.01 ± 0.22 | 46.13 ± 0.06 | 362 ± 49 | 46.66 ± 0.02 | 124 ± 11 |
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9.13 ± 0.30 (c) |
cid_357 | BL | 9.85 ± 0.31 | < 45.60 | < 108 | 45.25 ± 0.06 | 110 ± 11 | < 22.87 |
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8.46 ± 0.30 (d) |
cid_451 | NL | 11.21 ± 0.05 | 45.25 ± 0.17 (e) | 48 ± 19 | 46.44 ± 0.07 | 137 ± 12 |
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– |
cid_1205 | BL | 11.20 ± 0.10 | 46.16 ± 0.04 | 384 ± 33 | 45.75 ± 0.17 | 34 ± 6 |
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8.60 ± 0.30 (c) |
cid_2682 | NL | 11.03 ± 0.04 | < 45.54 | < 93 | 45.48 ± 0.10 | 36 ± 6 |
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– |
cid_247 | BL | 10.03 ± 0.20 | 45.73 ± 0.05 | 143 ± 15 | 45.49 ± 0.04 | 158 ± 13 | < 22.43 |
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8.17 ± 0.31 (c) |
cid_1215 | BL | 10.20 ± 0.08 | 45.96 ± 0.04 | 246 ± 24 | 45.73 ± 0.05 | 78 ± 9 |
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8.37 ± 0.30 (d) |
cid_467 | BL | 10.10 ± 0.29 | < 45.74 | < 147 | 46.53 ± 0.04 | 447 ± 21 |
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9.28 ± 0.31 (c) |
cid_852 | NL | 11.17 ± 0.02 | < 45.57 | < 100 | 45.50 ± 0.11 | 25 ± 5 |
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– |
cid_970 | NL | 10.38 ± 0.12 | < 45.66 | < 122 | 45.71 ± 0.04 | 287 ± 17 | < 22.25 |
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– |
cid_971 | NL | 10.60 ± 0.12 | – | < 96 (f) | 44.71 ± 0.24 | 33 ± 6 | < 23.68 |
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– |
cid_38 | NL | 11.01 ± 0.12 | < 45.98 | < 258 | 45.78 ± 0.04 | 159 ± 13 | < 22.95 |
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– |
lid_206 | BL | 10.30 ± 0.25 | – | 63 ± 27 (f) | 44.77 ± 0.12 | 40 ± 6 | < 22.55 |
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8.37 ± 0.30 (d) |
cid_1253 | NL | 10.99 ± 0.25 | 46.02 ± 0.30 | 280 ± 194 | 45.08 ± 0.18 | 36 ± 6 |
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– |
Notes. (1) Target ID; (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 (star formation only) 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.
Bolometric luminosities estimated from X-ray luminosities by using the relation of Duras et al. (2020).
BH masses from Menzel et al. (2016).
BH masses from Vietri et al. (2020).
BH masses from COSMOS or SDSS spectra estimated by following the method presented in Vietri et al. (2020).
FIR luminosity estimated by including in our SED fitting analysis ALMA Band 7 data from Lamperti et al. (in prep.). In Circosta et al. (2018) this value was an upper limit.
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