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Table 1

Average properties of the BAT AGN in our variability sample, as a function of the AGN class and the amount of intrinsic absorption.

Type z a F14−195 keV a ⟨Γ⟩ a SV a SV,14−24 keV b SV,35−100 keV b
[10-11 erg cm-2 s-1] [%] [%] [%]

Sey 1 0.033 (36) 6.4 ± 0.8 2.01 ± 0.02 16.5 ± 0.9 21 ± 2 (15) 13 ± 2
Sey 1.5 0.017 (17) 10 ± 2 1.92 ± 0.03 24 ± 1 32 ± 2 (11) 23 ± 2
Sey 2 0.016 (32) 10 ± 1 1.86 ± 0.03 19.9 ± 0.7 28 ± 1 (22) 16.2 ± 0.9
NLS1 0.019 (3) 11 ± 6 2.2 ± 0.1 15 ± 3 24 ± 4 (2) 9 ± 4

unabs Sey 0.031 (41) 6.7 ± 0.7 2.00 ± 0.02 18.5 ± 0.8 25 ± 2 (23) 17 ± 2
abs Sey 0.016 (46) 10 ± 1 1.90 ± 0.03 19.7 ± 0.6 28 ± 1 (26) 16.4 ± 0.8
CT Sey 0.011 (6) 13 ± 4 1.8 ± 0.1 16 ± 1 37 ± 6 (4) 9 ± 1

all Sey 0.023 (88) 8.5 ± 0.8 1.95 ± 0.02 19.3 ± 0.5 26.9 ± 0.9 (50) 16.7 ± 0.7
radio galaxies 0.033 (9) 22 ± 12 2.1 ± 0.2 24 ± 1 26 ± 2 (9) 26 ± 2
blazars/quasars 0.855 (13) 7 ± 3 2.0 ± 0.2 33 ± 2 36 ± 2 (9) 35 ± 2

Notes. In parentheses, the number of objects used for the given average value is indicated.

(a)

All objects in the sample have measured redshift and photon index (from a simple power law fit).

(b)

Only objects having variability measured in both the 14–24 and the 35–100 keV bands have been considered here.

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