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Table 1

Properties of the full sample with S/N > 15 and its subsamples.

Sample N sp N s N 2−12 N 5−8  ⟨ z ⟩   ⟨ log (L) ⟩   ⟨ NH,22 ⟩  N H,22  ⟨ S/N ⟩  α Σ6

(erg s-1) (1022 cm-2) (1022 cm-2) (eV)
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11) (12)

Full 100 54 181 623 40 863 1.34 43.74 1.48 0.08 29.8 0.35 119

Unabs 52 32 110 523 21 071 1.27 43.78 0.02 0.0 33.60 0.34 122
Abs 29 17 45 896 14 373 1.28 43.64 4.90 2.41 24.88 0.37 116

z < 1 39 20 72 672 18 148 0.64 43.21 1.61 0.17 30.0 0.35 95
z ≥ 1 61 34 108 951 22 715 1.80 44.07 1.39 0.04 28.8 0.35 134

Sey 61 33 91 511 20 987 0.91 43.35 1.35 0.11 26.2 0.34 108
QSO 39 21 90 111 19 876 2.02 44.34 1.68 0.04 34.1 0.36 138

Notes. Unabs and Abs subsamples have and and respectively; Sey and QSO subsample have and respectively (see text). Columns: (1) (sub)sample; (2) number of spectra; (3) number of sources; (4) number of net counts in 2–12 keV rest-frame; (5) number of net counts in 5–8 keV rest-frame; (6) average redshift; (7) logarithm of the average rest-frame 2–10 keV luminosity in units of erg s-1, corrected for Galactic and intrinsic absorption; (8) and (9) average and median of the intrinsic column density in 1022 cm-2; (10) average S/N of the (sub)sample between 2 and 12 keV rest-frame; (11) slope of the power-law dependence between the width of the simulated unresolved lines and their central energies Σ = Eα (see Sect. 3.3); (12) width at 6 keV of the simulated iron lines (see Sect. 3.3).

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