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Table 3:

Spectral fit of a cut-off power-law model for AGN with more complex IBIS/ISGRI spectra.
Name $N_{\rm H}$ $\Gamma_{\rm ISGRI}$ $E_{\rm C}$ $\chi_\nu^2$ (d.o.f.)
  $[10^{22}~\rm cm^{-2}]$   $[\rm keV]$  
Mrk 348 30 $0.9 {+0.4 \atop -0.6}$ $55 {+56 \atop -25}$ 0.91 (8)
NGC 4151 6.9 $1.60 {+0.06 \atop -0.07}$ $118 {+21 \atop
-13}$ 1.10 (9)
NGC 4388 27 $1.3 \pm 0.1$ $95 {+26 \atop -17}$ 0.34 (7)
NGC 4507 29 $1.15 {+0.28 \atop -0.13}$ $72 {+53 \atop
-22}$ 0.54 (8)
NGC 4593 0.02 $1.1 {+0.4 \atop -0.2}$ $48 {+114 \atop -9}$ 0.87 (7)
NGC 4945 400 $1.43 {+0.16 \atop -0.11}$ $127{+56 \atop
-26}$ 0.75 (8)
4U 1344-60 5 $1.11 {+0.29 \atop -0.09}$ $51 {+27 \atop
-12}$ 0.76 (7)
IC 4329A 0.42 $1.37 \pm 0.17$ $80 {+31 \atop -19}$ 1.50 (9)
Circinus Galaxy 360 $1.29 {+0.18 \atop -0.13}$ $33 {+6 \atop
-3}$ 1.03 (7)
GRS 1734-292 3.7 $1.50 \pm 0.10$ $54 {+8 \atop -7}$ 0.88 (8)
IGR J17488-3253 0.2 $0.74 {+0.33 \atop -0.12}$ $40 {+8 \atop
-3}$ 0.98 (7)
IGR J21247+5058 0.6 $1.19 {+0.13 \atop -0.19}$ $74 {+38 \atop
-28}$ 0.75 (8)

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