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Table 2.

Best-fit model parameters from CIGALE SED fitting.

Source (a) Survey Redshift (b) Red.χ2 AGN fraction Inclination log L 6 μ m AGN Mathematical equation: $ \log L_{6\,{\upmu}\mathrm{m}}^{\mathrm{AGN}} $(c) log N H IR Mathematical equation: $ \log N_{\mathrm{H}}^{\mathrm{IR}} $(d)



bayes best bayes best bayes best
hz414292 XXL-N 3.24 2.5 < 0.37 0.1 52 ± 8 50 45 . 3 0.5 + 0.2 Mathematical equation: $ 45.3_{-0.5}^{+0.2} $ 45.2 23 . 7 0.6 + 0.7 Mathematical equation: $ 23.7^{+0.7}_{-0.6} $
hz434324 XXL-N 3.16 1.5 < 0.40 0.2 64 ± 22 30 < 44.8 44.0 23 . 5 1.8 + 0.5 Mathematical equation: $ 23.5^{+0.5}_{-1.8} $
cdfs101 CDF-S 3.47 0.5 < 0.37 0.8 63 ± 18 50 44 . 5 0.8 + 0.3 Mathematical equation: $ 44.5_{-0.8}^{+0.3} $ 44.8 24.9 ± 1.0
cdfs337 CDF-S 3.6600 3.8 0.54 ± 0.19 0.5 75 ± 14 50 45 . 1 0.2 + 0.1 Mathematical equation: $ 45.1_{-0.2}^{+0.1} $ 44.9 24.2 ± 0.3
cdfs657 CDF-S 3.47 0.8 < 0.30 0.3 71 ± 19 70 < 44.1 43.9 24.0 ± 0.2
lid_1278 CCLS 3.01 2.0 0.51 ± 0.18 0.7 73 ± 11 70 45 . 0 0.2 + 0.1 Mathematical equation: $ 45.0_{-0.2}^{+0.1} $ 45.2 23 . 3 0.2 + 0.4 Mathematical equation: $ 23.3^{+0.4}_{-0.2} $
cid_965 CCLS 3.1780 0.4 0.73 ± 0.10 0.8 50 ± 1 50 45 . 41 0.05 + 0.04 Mathematical equation: $ 45.41_{-0.05}^{+0.04} $ 45.4 24 . 2 0.5 + 0.2 Mathematical equation: $ 24.2^{+0.2}_{-0.5} $
lid_439 CCLS 2.93 4.8 0.63 ± 0.17 0.5 76 ± 12 70 44 . 7 0.2 + 0.1 Mathematical equation: $ 44.7_{-0.2}^{+0.1} $ 44.8 23 . 6 0.6 + 0.13 Mathematical equation: $ 23.6^{+0.13}_{-0.6} $
cdfn158 CDF-N 3.19 2.4 0.35 ± 0.18 0.3 50 ± 4 50 45 . 5 0.2 + 0.1 Mathematical equation: $ 45.5_{-0.2}^{+0.1} $ 45.5 25 . 0 0.6 + 1.0 Mathematical equation: $ 25.0^{+1.0}_{-0.6} $
cdfn257 CDF-N 2.95 0.5 < 0.3 0.4 67 ± 19 50 44 . 1 0.8 + 0.3 Mathematical equation: $ 44.1_{-0.8}^{+0.3} $ 44.2 24 . 5 0.7 + 1.5 Mathematical equation: $ 24.5^{+1.5}_{-0.7} $

Notes. (a) Sources that remain high likelihood CTK (P(log NH > 24) > 0.8 after our SED analysis showed in boldface; (b) Bold values correspond to spectroscopic redshifts; (c) Decimal logarithm of the luminosity of the AGN component at 6 μm in C.G.S. units; (d) Decimal logarithm of the NH estimated with the IR-updated posteriors, following the method presented in Sect. 3.2. Errors and upper-limits correspond to 1-σ confidence intervals.

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