Table 5: Spectral fit with a broken power law model ( $\Gamma _{\rm soft}$, $\Gamma _{\rm hard}$, and $E_{\rm c}$ break point for the energy in keV), including the Galactic ( $N^{\rm Gal}_{\rm H}$) and intrinsic ( $N^{\rm in}_{\rm H}$) absorptions (expressed in 1020 cm-1). The unabsorbed fluxes are expressed in 10-12 erg s-1 cm-2. In parentheses are reported the luminosities (expressed in 1044 erg s-1). The last column reports the flux ratio in the 0.3-2 keV and 0.3-10 keV energy bands. For PG 1114+445, two strong absorption edges are required (see values in Table 6).
Source $N^{\rm in}_{\rm H}$ $\Gamma _{\rm soft}$ $\Gamma _{\rm hard}$ $E_{\rm c}$ $\chi^{2}$/d.o.f. P($\chi^{2}$) F0.3-10 (L) F2-10 (L) $\frac{\rm0.3-2~keV}{0.3-10~\rm keV}$

I Zw1		 5.0 $\pm$ 0.6 2.61 $\pm$ 0.10 2.37 $\pm$ 0.02 0.67 $\pm$ 0.05 642.0/495 0 28.3 (2.1) 8.4 (0.63) 70$\%$
PG 0804+761 <2.8 $\rm 2.47^{+0.19}_{-0.10}$ $\rm 2.16^{+0.04}_{-0.09}$ $\rm 1.26^{+0.50}_{-0.12}$ 489.0/475 31.8 32. (6.6) 11. (2.2) 66$\%$
PG 0947+396 <0.7 2.41 $\pm$ 0.03 1.75 $\pm$ 0.09 2.28 $\pm$ 0.23 462.9/484 74.8 4.6 (4.3) 1.8 (1.5) 61$\%$
PG 0953+414 <0.6 $\rm 2.60^{+0.05}_{-0.02}$ 2.02 $\pm$ 0.07 1.77 $\pm$ 0.19 410.9/380 13.2 9.3 (12.3) 3.0 (3.7) 68$\%$
PG 1048+342 <1.2 $\rm 2.40^{+0.11}_{-0.03}$ 1.80 $\pm$ 0.07 $\rm 1.80^{+0.21}_{-0.17}$ 428.3/386 6.8 3.3 (1.9) 1.4 (0.76) 58$\%$
PG 1114+445 <1.5 $\rm 1.56^{+0.09}_{-0.04}$ 1.53 $\pm$ 0.03 2.0 (f) 481.4/410 0.9 3.1 (1.2) 2.3 (0.89) 26$\%$
PG 1115+407 <0.8 $\rm 2.85^{+0.06}_{-0.02}$ 2.19 $\pm$ 0.10 $\rm 2.04^{+0.24}_{-0.20}$ 357.0/406 96.2 5.3 (2.9) 1.2 (0.60) 77$\%$
PG 1116+215 <1.9 $\rm 2.72^{+0.18}_{-0.03}$ 2.17 $\pm$ 0.11 $\rm 1.76^{+0.32}_{-0.41}$ 396.3/401 55.7 12. (8.3) 3.2 (2.1) 73$\%$
PG 1202+281 <0.5 2.29 $\pm$ 0.04 1.71 $\pm$ 0.06 $\rm 1.76^{+0.24}_{-0.16}$ 413.8/375 8.2 7.8 (4.4) 3.6 (1.9) 55$\%$
PG 1244+026 12.1 $\pm$ 0.1 3.77 $\pm$ 0.11 2.51 $\pm$ 0.10 $\rm 1.81^{+0.12}_{-0.09}$ 523.8/403 0 29. (1.4) 2.2 (0.099) 92$\%$
PG 1307+085 <7.0 $\rm 2.86^{+0.47}_{-0.22}$ 1.52 $\pm$ 0.06 0.93 $\pm$ 0.06 360.4/338 19.3 3.4 (1.7) 1.9 (0.87) 44$\%$
PG 1309+355 <3.4 $\rm 2.92^{+0.34}_{-0.13}$ 1.73 $\pm$ 0.05 0.78 $\pm$ 0.05 269.1/301 90.7 1.4 (1.0) 0.71 (0.48) 49$\%$
PG 1322+659 <2.8 $\rm 3.01^{+0.24}_{-0.04}$ $\rm 2.18^{+0.14}_{+0.11}$ $\rm 1.62^{+0.19}_{-0.25}$ 337.3/336 47.0 5.8 (3.8) 1.3 (0.77) 78$\%$
PG 1352+183 <0.7 2.65 $\pm$ 0.04 1.93 $\pm$ 0.10 $\rm 2.00^{+0.17}_{-0.23}$ 485.2/458 18.3 6.0 (3.0) 1.9 (0.88) 68$\%$
PG 1402+261 <2.8 $\rm 2.91^{+0.13}_{-0.09}$ $\rm 2.18^{+0.08}_{-0.13}$ $\rm 1.73^{+0.35}_{-0.17}$ 424.1/384 7.7 7.7 (4.7) 1.8 (1.0) 77$\%$
Mrk 1383 <1.2 $\rm 2.62^{+0.11}_{-0.02}$ 1.96 $\pm$ 0.10 $\rm 1.91^{+0.25}_{-0.28}$ 457.4/460 52.6 23. (3.6) 7.5 (1.1) 67$\%$
PG 1427+480 <1.6 $\rm 2.53^{+0.10}_{-0.03}$ 1.87 $\pm$ 0.07 $\rm 1.92^{+0.17}_{-0.22}$ 495.5/488 39.8 2.8 (3.0) 1.0 (1.0) 64$\%$
Mrk 478 2.2 $\pm$ 1.1 3.25 $\pm$ 0.10 2.38 $\pm$ 0.06 1.56 $\pm$ 0.10 422.3/465 92.2 17. (2.2) 2.7 (0.33) 84$\%$
PG 1512+370 <0.9 2.31 $\pm$ 0.04 1.78 $\pm$ 0.05 $\rm 1.81^{+0.16}_{-0.13}$ 473.1/479 56.7 4.3 (13.) 1.9 (5.3) 56$\%$
Mrk 876 <2.3 $\rm 2.56^{+0.19}_{-0.06}$ $\rm 1.85^{+0.08}_{-0.10}$ $\rm 1.45^{+0.21}_{-0.13}$ 344.6/322 18.5 12.9 (4.5) 5.2 (1.7) 60$\%$
PG 1626+554 <0.8 2.41 $\pm$ 0.05 1.99 $\pm$ 0.12 $\rm 1.72^{+0.43}_{-0.52}$ 388.0/388 49.0 8.3 (3.0) 3.1 (1.1) 63$\%$


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