Table A.3: Fit results with the broken power law model. Columns: (1) source name; (2) absorbing column density [1020 cm-2]; (3) low energy photon index of the power law; (4) high energy photon index; (5) break energy [keV]; (6) normalization of the power law model [10-2 ph cm-2 s-1 keV-1 at 1 keV]; (7) reduced $\chi ^2$ and degrees of freedom; (8) observed flux in the 0.4-10 keV energy band [10-11 erg cm-2 s-1]; (9) intrinsic luminosity in the 0.4-10 keV energy band rest frame [1045 erg s-1]; (10) Ftest probability [%]; fit with probability below 90% are not reported. 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 $N_{{\rm H}}$ $\Gamma _1$ $\Gamma _2$ $E_{\rm break}$ A $\tilde{\chi}^2$/d.o.f. F L Ftest
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10)
0219+428 Gal. $\rm 2.91_{-0.08}^{+0.12}$ $\rm 2.23_{-0.09}^{+0.10}$ $1.3\pm 0.2$ $0.067\pm 0.003$ 1.05/291 0.24 3.0 >99.99
AO 0235+164 Gal. $2.33\pm 0.04$ $2.1\pm 0.1$ $\rm 3.3_{-0.5}^{+0.7}$ $0.276\pm 0.006$ 0.96/616 0.99 69 >99.99
PKS 0521-365 Gal. $1.95\pm 0.03$ $1.74\pm 0.03$ $\rm 1.5_{-0.2}^{+0.3}$ $0.227\pm 0.003$ 1.05/1200 1.3 $9.4\times 10^{-4}$ 99.97
S5  0716+714a Gal. $2.70\pm 0.02$ $\rm 1.98_{-0.09}^{+0.08}$ $\rm 2.3_{-0.1}^{+0.2}$ $0.293\pm 0.003$ 1.06/417 1.1 >15.7 >99.99
S5 0836+710 Gal. $1.25\pm 0.03$ $1.375\pm 0.007$ $\rm 1.01_{-0.08}^{+0.15}$ $0.529\pm 0.006$ 1.07/2271 4.8 860 -
Mkn 421b Gal. $2.573\pm 0.008$ $\rm 2.79_{-0.08}^{+0.17}$ $\rm 4.2_{-0.7}^{+1.0}$ $6.97\pm 0.02$ 0.96/1025 26.1 0.578 99.97
  Gal. $2.340\pm 0.004$ $2.73\pm 0.04$ $4.0\pm 0.2$ $22.9\pm 0.4$ 1.06/1490 91.3 2.00 >99.99
  Gal. $\rm 2.378_{-0.005}^{+0.004}$ $\rm 2.96_{-0.10}^{+0.08}$ $\rm 4.7_{-0.3}^{+0.2}$ $22.6\pm 0.4$ 1.02/1429 89.1 1.95 >99.99
  Gal. $2.312\pm 0.007$ $\rm 2.68_{-0.05}^{+0.07}$ $4.4\pm 0.3$ $16.4\pm 0.7$ 0.99/1446 66.7 1.45 >99.99
  Gal. $\rm 2.59_{-0.02}^{+0.01}$ $2.81\pm 0.02$ $\rm 2.2_{-0.2}^{+0.1}$ $\rm 11.5_{-0.8}^{+0.7}$ 1.08/1177 41.8 0.929 >99.99
  Gal. $2.300\pm 0.007$ $2.51\pm 0.02$ $2.2\pm 0.1$ $14.1\pm 0.4$ 0.99/1306 56.3 1.23 >99.99
PKS  1127-145c $\rm 12_{-1}^{+2}$ $\rm 1.40_{-0.05}^{+0.08}$ $1.22\pm 0.06$ $\rm 2.7_{-0.8}^{+1.0}$ $\rm0.127_{-0.004}^{+0.006}$ 1.00/888 1.2 61.0 99.58
ON 231 Gal. $2.74\pm 0.02$ $\rm 2.3_{-0.4}^{+0.3}$ $\rm 4.2_{-1.1}^{+0.9}$ $0.140\pm 0.002$ 1.07/652 0.51 0.16 94.50
3C 273 Gal. $1.943\pm 0.009$ $1.697\pm 0.009$ $1.48\pm 0.06$ $2.073\pm 0.008$ 1.13/1596 12.7 8.7 >99.99
  Gal. $1.97\pm 0.01$ $1.65\pm 0.01$ $1.43\pm 0.08$ $1.97\pm 0.01$ 1.03/1399 12.5 8.6 >99.99
  Gal. $1.96\pm 0.01$ $1.67\pm 0.01$ $1.35\pm 0.08$ $1.91\pm 0.01$ 1.00/1392 12.1 8.3 >99.99
  Gal. $1.92\pm 0.01$ $1.654\pm 0.009$ $1.37\pm 0.05$ $1.911\pm 0.008$ 0.97/1645 12.2 8.4 >99.99
  Gal. $2.121\pm 0.007$ $1.676\pm 0.008$ $1.45\pm 0.03$ $2.604\pm 0.009$ 1.10/1709 15.7 11.0 >99.99
  Gal. $2.00\pm 0.02$ $1.72\pm 0.02$ $\rm 1.4_{-0.1}^{+0.2}$ $3.06\pm 0.03$ 1.00/800 18.4 12.7 >99.99
  Gal. $1.94\pm 0.03$ $1.67\pm 0.03$ $1.5\pm 0.2$ $2.95\pm 0.03$ 0.95/804 18.4 12.6 >99.99
  Gal. $1.97\pm 0.03$ $\rm 1.79_{-0.04}^{+0.03}$ $\rm 1.4_{-0.2}^{+0.4}$ $2.29\pm 0.03$ 1.01/678 13.1 9.09 >99.99
  Gal. $2.09\pm 0.02$ $1.81\pm 0.03$ $1.6\pm 0.1$ $3.39\pm 0.03$ 0.97/788 18.6 13.2 >99.99
  Gal. $2.16\pm 0.02$ $\rm 1.83_{-0.03}^{+0.02}$ $\rm 1.4_{-0.1}^{+0.2}$ $2.80\pm 0.03$ 0.99/897 15.1 10.8 >99.99
  Gal. $2.13\pm 0.02$ $\rm 1.81_{-0.05}^{+0.04}$ $\rm 1.7_{-0.2}^{+0.3}$ $2.88\pm 0.03$ 0.96/709 15.4 10.9 >99.99
  Gal. $2.05\pm 0.02$ $1.76\pm 0.03$ $1.8\pm 0.2$ $3.51\pm 0.03$ 1.02/824 19.5 13.7 >99.99
  Gal. $2.02\pm 0.02$ $\rm 1.82_{-0.07}^{+0.03}$ $\rm 1.9_{-0.3}^{+0.6}$ $3.05\pm 0.02$ 1.00/906 16.4 11.6 >99.99
  Gal. $2.02\pm 0.02$ $1.70\pm 0.03$ $\rm 1.7_{-0.1}^{+0.2}$ $2.26\pm 0.02$ 1.02/875 13.2 9.20 >99.99
  Gal. $\rm 2.00_{-0.01}^{+0.02}$ $1.76\pm 0.02$ $\rm 1.5_{-0.1}^{+0.2}$ $1.94\pm 0.01$ 1.03/1158 11.2 7.8 >99.99
Cen A                 -
                  -
PKS 1334-127 Gal. $\rm 1.57_{-0.24}^{+0.08}$ $1.78\pm 0.03$ $1.0\pm 0.3$ $\rm0.077_{-0.003}^{+0.012}$ 0.92/608 0.43 4.8 92.31
PKS 1406-076                 81.60
                  56.30
NGC 6251 $14\pm 1$ $\rm 2.11_{-0.06}^{+0.08}$ $1.78\pm 0.07$ $\rm 2.5_{-0.4}^{+0.3}$ $0.141\pm 0.004$ 1.00/810 0.59 0.010 >99.99
PKS 1830-211 $\rm 62_{-6}^{+5}$ $\rm0.93_{-0.10}^{+0.08}$ $\rm 1.42_{-0.05}^{+0.10}$ $\rm 3.6_{-0.5}^{+0.4}$ $0.11\pm 0.01$ 0.83/598 1.38 270 >99.99
  $62\pm 3$ $\rm0.89_{-0.09}^{+0.06}$ $1.29\pm 0.04$ $3.1\pm 0.3$ $\rm0.103_{-0.08}^{+0.06}$ 0.97/1660 1.31 243 >99.99
  $64\pm 3$ $1.06\pm 0.04$ $\rm 1.41_{-0.09}^{+0.12}$ $\rm 4.7_{-0.4}^{+0.5}$ $0.108\pm 0.06$ 1.00/1166 1.20 248 >99.99
PKS  2155-304b Gal. $2.588\pm 0.005$ $\rm 2.73_{-0.08}^{+0.18}$ $\rm 4.4_{-1.1}^{+1.4}$ $3.861\pm 0.008$ 1.01/1265 14.3 5.70 >99.99
  Gal. $\rm 2.773_{-0.006}^{+0.007}$ $\rm 2.88_{-0.03}^{+0.06}$ $\rm 2.8_{-0.4}^{+0.7}$ $3.246\pm 0.007$ 0.98/1066 11.6 4.74 >99.99
  Gal. $2.845\pm 0.006$ $3.0\pm 0.1$ $\rm 4.3_{-1.2}^{+0.8}$ $2.620\pm 0.007$ 1.02/990 9.31 3.86 99.67
  Gal. $2.783\pm 0.006$ $2.96\pm 0.04$ $\rm 2.4_{-0.2}^{+0.3}$ $5.75\pm 0.01$ 0.97/1130 20.3 8.35 >99.99
  Gal. $2.75\pm 0.03$ $\rm 2.70_{-0.02}^{+0.01}$ $\rm 1.0_{-0.1}^{+0.5}$ $2.74\pm 0.02$ 0.99/885 10.0 4.10 96.01
                  -
                  89.10
                  -
                  85.00
a Only MOS1+MOS2, since the PN was set in TIMING. Lower limit of luminosity calculated for z=0.5.
b Fit in the 0.6-10 keV energy range and extrapolation to 0.4 keV for flux and luminosity calculations.
c Additional redshifted absorber (wa*zwa(bknpo) model in xspec) along the line of sight.

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