Table 10: Spectral fit with absorbed compTT+power law. For the COMPTT component model, the soft photon temperature ( ${\it kT}^{\rm photon}_{1}$) is fixed to Tmax (Col. 1 of Table 9). ${\it kT}^{\rm plasma}$ is expressed in keV. $\tau $ corresponds to the plasma optical depth. The fits include the Galactic ( $N^{\rm Gal}_{\rm H}$) and intrinsic ( $N^{\rm in}_{\rm H}$) absorptions. Column densities are 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. (a) one or two absorption edges are added to the continuum model due to the presence of a WA. (b) a Fe K line is added (either a Gaussian line or a LAOR line).
Source $N^{\rm in}_{\rm H}$ $kT^{\rm plasma}$ $\tau_{1}$ $\Gamma$ $\chi^{2}$/d.o.f. F0.3-10 (L) F2-10 (L)   $\frac{\rm0.3-2~\rm keV}{0.3-10~\rm keV}$ 

I Zw1(a,b)		 10.5 $\pm$ 2.6 0.22 $\pm$ 0.05 $\rm 14.7^{+2.2}_{-1.3}$ 2.33 $\pm$ 0.03 525.7/490 36.3 (2.8) 8.6 (0.64) 76$\%$
PG 0804+761(a,b) $\rm 3.9^{+7.2}_{-3.1}$ $\rm 2.8^{+3.1}_{-1.4}$ $\rm 3.5^{+2.1}_{-1.1}$ $\rm 1.53^{+0.32}_{-0.17}$ 462.5/470 30.5 (6.1) 11.4 (2.3) 63$\%$
PG 0947+396(a,b) <3.3 0.32 $\pm$ 0.06 $\rm 15.6^{+0.8}_{-2.0}$ 1.76 $\pm$ 0.07 440.1/479 4.6 (4.2) 1.8 (1.6) 61$\%$
PG 0953+414 <2.0 $\rm0.29^{+0.10}_{-0.06}$ $\rm 13.8^{+0.5}_{-1.0}$ 1.98 $\pm$ 0.05 408.6/379 9.1 (11.9) 3.0 (3.7) 67$\%$
PG 1048+342(b) <1.8 $\rm0.25^{+0.09}_{-0.06}$ $\rm 16.6^{+0.8}_{-1.5}$ 1.82 $\pm$ 0.06 417.4/383 3.2 (1.9) 1.3 (0.74) 60$\%$
PG 1114+445(a,b) $\rm 5.2^{+2.5}_{-3.5}$ $\rm 3.1^{+9.7}_{-2.2}$ $\rm 6.7^{+3.2}_{-4.0}$ 1.51 (f) 214.6/236 3.3 (1.3) 2.3 (0.92) 30$\%$
PG 1115+407(a,b) <7.2 $\rm0.17^{+0.08}_{-0.04}$ $\rm 19.2^{+5.4}_{-3.4}$ 2.40 $\pm$ 0.06 333.2/399 5.8 (3.1) 1.2 (0.60) 79$\%$
PG 1116+215(a,b) <11.8 $\rm0.25^{+0.18}_{-0.07}$ $\rm 13.1^{+3.7}_{-2.1}$ 2.23 $\pm$ 0.08 370.3/396 14.8 (11.0) 3.2 (2.1) 78$\%$
PG 1202+281(a) <6.7 0.24 $\pm$ 0.07 $\rm 21.2^{+1.8}_{-4.8}$ 1.68 $\pm$ 0.04 396.9/372 7.5 (4.2) 3.6 (1.9) 52$\%$
PG 1244+026(b) <2.1 0.18 $\pm$ 0.02 $\rm 28.7^{+2.5}_{-4.0}$ 2.40 $\pm$ 0.08 426.8/400 12.4 (0.57) 2.1 (0.098) 83$\%$
PG 1307+085(a) 5.4 $\pm$ 4.2 0.10 $\pm$ 0.02 >44 1.46 $\pm$ 0.03 350.1/337 3.4 (1.6) 1.9 (0.87) 44$\%$
PG 1309+355(a,b) <13.1 $\rm0.13^{+0.08}_{-0.03}$ >23.4 $\rm 1.78^{+0.09}_{-0.06}$ 244.4/295 1.4 (1.0) 0.72 (0.48) 49$\%$
PG 1322+659 <4.3 0.17 $\pm$ 0.05 $\rm 22.4^{+1.7}_{-3.7}$ 2.21 $\pm$ 0.07 327.1/335 5.3 (3.4) 1.3 (0.77) 76$\%$
PG 1352+183(a) <6.8 0.25 $\pm$ 0.06 $\rm 17.6^{+0.9}_{-3.0}$ 1.90 $\pm$ 0.08 476.0/455 5.7 (2.8) 1.9 (0.88) 67$\%$
PG 1402+261(b) <3.1 $\rm0.25^{+0.11}_{-0.06}$ $\rm 14.2^{+0.6}_{-1.7}$ 2.20 $\pm$ 0.08 407.5/381 7.3 (4.4) 1.8 (1.0) 75$\%$
Mrk 1383(b) <1.0 0.20 $\pm$ 0.05 $\rm 19.1^{+0.9}_{-1.2}$ 2.02 $\pm$ 0.05 438.8/457 23.2 (3.5) 7.5 (1.1) 68$\%$
PG 1427+480 <4.8 $\rm0.27^{+0.08}_{-0.05}$ $\rm 16.0^{+0.7}_{-2.4}$ 1.86 $\pm$ 0.05 494.9/487 2.7 (2.8) 1.0 (1.0) 63$\%$
Mrk 478 <5.1 0.22 $\pm$ 0.05 13.6 $\pm$ 1.3 2.29 $\pm$ 0.06 416.4/464 15.8 (2.0) 2.7 (0.33) 83$\%$
PG 1512+370(b) <6.5 $\rm0.44^{+0.72}_{-0.12}$ $\rm 10.9^{+0.6}_{-2.4}$ 1.74 $\pm$ 0.08 468.6/476 4.3 (13.5) 1.9 (5.4) 56$\%$
Mrk 876(a) <4.0 0.14 $\pm$ 0.06 >37.4 1.86 $\pm$ 0.06 327.4/320 11.8 (4.0) 5.1 (1.7) 57$\%$
PG 1626+554 <6.9 $\rm0.52^{+7.84}_{-0.30}$ $\rm 9.4^{+0.7}_{-2.2}$ 1.85 $\pm$ 0.17 385.9/387 8.0 (2.9) 3.1 (1.1) 61$\%$


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