Table 1: Sources detected in the IBIS/ISGRI field of S5 0716+714.
Object AGN type z CR^a Flux^b Range^c $\Gamma_1^d$ $\Gamma_2^d$ E_b^e $\chi^2$ d.o.f. $\Gamma_{\rm PDS}^f$

S5 0716+714 BL Lac ... $0.36 \pm 0.07^g$ 3.1 30-60 ... ... ... ... ... $1.6 \div 2.0$

S5 0836+710 FSRQ 2.172 $0.54 \pm 0.05$ 4.6 20-100 $1.3 \pm 0.3^h$ ... ... 4.1 5 $1.31 \pm 0.03$

Mkn 6 Sy 1.5 0.019 $0.49 \pm 0.06$ 4.6 20-100 1.5^+0.5_-0.4 ... ... 3.7 3 $1.8 \pm 0.2$

Mkn 3 Sy 2 0.013 $0.82 \pm 0.05$ 7.4 20-100 1.3ⁱ >2.5 $80 \pm 20^h$ 2.5 3 $1.8 \pm 0.1$

^a IBIS/ISGRI count rate in the detection energy range (Col. 6), in counts s^-1.

^b Fitted flux in the detection energy range (Col. 6), in 10^-11 erg s^-1 cm^-2. Calibration uncertainties are $\sim$ 10%.

^c Energy interval to which count rates (Col. 4) and fluxes (Col. 5) are referred, in keV.

^d Photon index: $f_E \propto E^{-\Gamma}$ .

^e Break energy, in keV.

^f Photon index measured with the BeppoSAX PDS at previous epochs.

^g Uncertainties on the count rates are 1 $\sigma$ .

^h Uncertainties on the photon indices and break energy are 1.6 $\sigma$ .

ⁱ $\Gamma_1$ has been frozen to the index of the single power-law which best fits the spectrum below 100 keV, $\Gamma = 1.3 \pm 0.4$ .

**Table 1:** Sources detected in the IBIS/ISGRI field of S5 0716+714.
Object	AGN type	z	CR^a	Flux^b	Range^c	$\Gamma_1^d$	$\Gamma_2^d$	E_b^e	$\chi^2$	d.o.f.	$\Gamma_{\rm PDS}^f$
S5 0716+714	BL Lac	...	$0.36 \pm 0.07^g$	3.1	30-60	...	...	...	...	...	$1.6 \div 2.0$
S5 0836+710	FSRQ	2.172	$0.54 \pm 0.05$	4.6	20-100	$1.3 \pm 0.3^h$	...	...	4.1	5	$1.31 \pm 0.03$
Mkn 6	Sy 1.5	0.019	$0.49 \pm 0.06$	4.6	20-100	1.5^+0.5_-0.4	...	...	3.7	3	$1.8 \pm 0.2$
Mkn 3	Sy 2	0.013	$0.82 \pm 0.05$	7.4	20-100	1.3ⁱ	>2.5	$80 \pm 20^h$	2.5	3	$1.8 \pm 0.1$

Source LaTeX | All tables | In the text

	1 Introduction
	2 Observations, data analysis and results
	3 Discussion
	References

^a IBIS/ISGRI count rate in the detection energy range (Col. 6), in counts s^-1.
^b Fitted flux in the detection energy range (Col. 6), in 10^-11 erg s^-1 cm^-2. Calibration uncertainties are $\sim$ 10%.
^c Energy interval to which count rates (Col. 4) and fluxes (Col. 5) are referred, in keV.
^d Photon index: $f_E \propto E^{-\Gamma}$ .
^e Break energy, in keV.
^f Photon index measured with the BeppoSAX PDS at previous epochs.
^g Uncertainties on the count rates are 1 $\sigma$ .
^h Uncertainties on the photon indices and break energy are 1.6 $\sigma$ .
ⁱ $\Gamma_1$ has been frozen to the index of the single power-law which best fits the spectrum below 100 keV, $\Gamma = 1.3 \pm 0.4$ .