Table A.2: Fit results with single powerl law model. Columns: (1) Source name; (2) absorbing column density [1020 cm-2]; (3) photon index of the power law; (4) normalization of the power law model [10-2 ph cm-2 s-1 keV-1 at 1 keV]; (5) reduced $\chi ^2$ and degrees of freedom; (6) observed flux in the 0.4-10 keV energy band [10-11 erg cm-2 s-1]; (7) intrinsic luminosity in the 0.4-10 keV energy band rest frame [1045 erg s-1]. The uncertainties in the parameter estimates are at the $90\%$ confidence limits for 1 parameter. For $N_{{\rm H}}={\rm Gal}$, it means that the absorption column has been fixed to the Galactic value.
Name $N_{{\rm H}}$ $\Gamma $ A $\tilde{\chi}^2$/d.o.f. F L
(1) (2) (3) (4) (5) (6) (7)
0219+428 Gal. $2.60\pm 0.04$ $0.183\pm 0.007$ 1.29/293 0.21 2.6
AO 0235+164 Gal. $2.28\pm 0.02$ $1.22\pm 0.04$ 0.99/618 0.96 66
PKS 0521-365 Gal. $1.847\pm 0.009$ $0.231\pm 0.002$ 1.15/1202 1.2 $9.0\times 10^{-4}$
S5  0716+714a Gal. $2.58\pm 0.02$ $0.294\pm 0.003$ 1.74/419 1.0 >14.2
S5  0836+710b $14\pm 3$ $1.379\pm 0.007$ $2.62\pm 0.04$ 1.07/2272 4.8 902
Mkn 421c $2.3\pm 0.3$ $2.61\pm 0.01$ $7.74\pm 0.09$ 0.97/1026 26.0 0.59
  $3.5\pm 0.2$ $2.438\pm 0.006$ $26.3\pm 0.1$ 1.20/1491 90.6 2.12
  $3.1\pm 0.2$ $2.457\pm 0.006$ $25.6\pm 0.1$ 1.29/1430 88.8 2.05
  $3.1\pm 0.2$ $2.373\pm 0.007$ $18.3\pm 0.1$ 1.12/1447 66.1 1.51
  $4.6\pm 0.2$ $2.73\pm 0.01$ $13.5\pm 0.1$ 1.16/1178 40.6 1.02
  $3.7\pm 0.2$ $2.43\pm 0.01$ $16.3\pm 0.1$ 1.03/1307 56.0 1.31
PKS  1127-145d $\rm 12_{-1}^{+2}$ $1.31\pm 0.02$ $0.34\pm 0.01$ 1.01/890 1.1 59.2
ON 231 $2.5\pm 0.6$ $2.77\pm 0.04$ $0.186\pm 0.005$ 1.07/653 0.50 0.16
3C 273 Gal. $1.829\pm 0.004$ $2.788\pm 0.007$ 1.82/1598 12.2 8.4
  Gal. $1.819\pm 0.005$ $2.68\pm 0.01$ 1.71/1401 11.8 8.2
  Gal. $1.812\pm 0.005$ $2.603\pm 0.009$ 1.53/1394 11.5 8.0
  Gal. $1.8\pm 0.2$ $2.599\pm 0.004$ 2.08/1647 11.5 8.0
  Gal. $1.9\pm 0.2$ $3.634\pm 0.004$ 4.22/1711 14.5 10.2
  Gal. $1.87\pm 0.01$ $4.18\pm 0.03$ 1.24/802 17.4 12.2
  Gal. $1.82\pm 0.01$ $3.97\pm 0.03$ 1.15/806 17.5 12.1
  Gal. $1.89\pm 0.01$ $3.09\pm 0.02$ 1.08/680 12.7 8.90
  Gal. $1.98\pm 0.01$ $4.67\pm 0.03$ 1.21/790 17.7 12.6
  Gal. $2.019\pm 0.009$ $3.92\pm 0.02$ 1.37/899 14.3 10.3
  Gal. $2.02\pm 0.01$ $3.99\pm 0.03$ 1.23/711 14.5 10.4
  Gal. $1.950\pm 0.009$ $4.78\pm 0.03$ 1.27/826 18.5 13.2
  Gal. $1.963\pm 0.008$ $4.13\pm 0.02$ 1.12/908 15.8 11.2
  Gal. $1.901\pm 0.009$ $3.07\pm 0.02$ 1.33/877 12.5 8.77
  Gal. $1.899\pm 0.006$ $2.64\pm 0.01$ 1.32/1160 10.7 7.54
Cen Ae $1400\pm 200$ $2.2\pm 0.1$ $\rm 22_{-5}^{+7}$ 0.97/668 16.9 $3.0\times 10^{-4}$
  $1800\pm 300$ $2.3\pm 0.2$ $\rm 29_{-9}^{+14}$ 0.97/340 18.5 $3.3\times 10^{-4}$
PKS 1334-127 $6.7\pm 0.9$ $1.80\pm 0.04$ $0.171\pm 0.009$ 0.93/609 0.43 5.1
PKS 1406-076 Gal. $1.58\pm 0.07$ $\rm0.060_{-0.006}^{+0.007}$ 0.79/90 0.10 10.5
  Gal. $1.6\pm 0.1$ $\rm0.056_{-0.007}^{0.009}$ 0.94/49 0.094 9.78
NGC 6251 $\rm 11.6_{-0.7}^{+0.8}$ $1.94\pm 0.03$ $0.134\pm 0.004$ 1.04/812 0.577 $9.6\times 10^{-3}$
PKS  1830-211d $350\pm 50$ $\rm 1.17_{-0.05}^{+0.03}$ $\rm0.62_{-0.08}^{+0.07}$ 0.90/600 1.42 322
  $240\pm 10$ $1.14\pm 0.02$ $0.54\pm 0.03$ 1.04/1662 1.34 290
  $220\pm 10$ $1.13\pm 0.03$ $0.47\pm 0.03$ 1.04/1168 1.22 261
PKS  2155-304c $1.6\pm 0.2$ $2.592\pm 0.009$ $5.12\pm 0.04$ 1.02/1266 14.4 5.71
  $2.2\pm 0.2$ $2.81\pm 0.01$ $4.49\pm 0.04$ 1.00/1067 11.6 4.87
  $1.9\pm 0.3$ $2.86\pm 0.01$ $3.61\pm 0.04$ 1.03/991 9.32 3.90
  $3.2\pm 0.2$ $2.868\pm 0.009$ $8.23\pm 0.06$ 1.01/1131 20.2 8.89
  $1.4\pm 0.3$ $2.70\pm 0.01$ $3.68\pm 0.05$ 0.99/886 10.0 4.02
  $3.0\pm 0.3$ $2.89\pm 0.01$ $2.81\pm 0.04$ 0.87/880 6.90 3.03
  Gal. $2.96\pm 0.01$ $2.40\pm 0.01$ 0.95/614 6.17 2.60
  $2.5\pm 0.5$ $3.08\pm 0.02$ $2.80\pm 0.05$ 0.88/625 6.83 3.04
  $2.9\pm 0.4$ $2.98\pm 0.02$ $3.77\pm 0.05$ 1.10/831 9.14 4.07
a Only MOS1+MOS2, since the PN was set in TIMING. Lower limit of luminosity calculated for z=0.5.
b Additional absorber placed at the redshift of the source (wa*zwa(zpo) model in xspec).
c Fit in the 0.6-10 keV energy range and extrapolation to 0.4 keV for flux and luminosity calculations.
d Additional redshifted absorber (wa*zwa(zpo) model in xspec) along the line of sight.
e Fit in the 4-10 keV energy range, without 6-8 keV energy band, because of complex features in the low energy part and in the iron emission line complex.

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