Table 9: Spectral fit with an absorbed black body spectrum of an accretion disk ( DISKPN, ${\it kT}_{\rm diskpn}$) combined with a power law model. $T^{\rm max}_{\rm disk}$ (in eV) represents the maximal values of the disk temperature for a standard $\alpha $ thin accretion disk at 3 $R_{\rm S}$. ${\it kT}_{\rm diskpn}$ is expressed in eV. (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		 $T^{\rm max}_{\rm disk}$ ${\it kT}_{\rm diskpn}$ $\Gamma$ $\chi^{2}$/d.o.f.

I Zw1(a,b)		39 200 $\pm$ 25 2.33 $\pm$ 0.03 540.0/493
PG 0804+761(a,b)15 $\rm 159^{+30}_{-23}$ 2.22 $\pm$ 0.07 464.1/468
PG 0947+396(a,b)11 241 $\pm$ 15 1.88 $\pm$ 0.06 451.0/480
PG 0953+41418 174 $\pm$ 8 2.12 $\pm$ 0.04 421.9/380
PG 1048+342(b)15 183 $\pm$ 11 1.91 $\pm$ 0.05 423.2/384
PG 1115+407(a,b)24 172 $\pm$ 14 2.40 $\pm$ 0.07 353.1/402
PG 1116+215(a,b)13 $\rm 175^{+17}_{-26}$ 2.30 $\pm$ 0.07 375.8/397
PG 1202+281(a)14 $\rm 223^{+14}_{-17}$ 1.72 $\pm$ 0.05 396.4/373
PG 1244+026(b)73 197 $\pm$ 11 2.39 $\pm$ 0.10 427.5/401
PG 1307+085(a)9 $\rm 142^{+41}_{-19}$ 1.55 $\pm$ 0.07 338.6/336
PG 1309+355(a,b)16 $\rm 144^{+39}_{-26}$ 1.78 $\pm$ 0.08 244.4/296
PG 1322+65919 149 $\pm$ 8 2.28 $\pm$ 0.07 226.3/336
PG 1352+183(a)15 201 $\pm$ 12 2.04 $\pm$ 0.08 478.8/456
PG 1402+261(b)31 $\rm 151^{+11}_{-17}$ 2.53 $\pm$ 0.09 400.4/381
Mrk 1383(b)7 160 $\pm$ 8 2.09 $\pm$ 0.05 442.8/458
PG 1427+48021 190 $\pm$ 9 1.98 $\pm$ 0.05 505.9/488
Mrk 47835 138 $\pm$ 4 2.48 $\pm$ 0.05 455.0/465
PG 1512+370(b)9 210 $\pm$ 19 1.90 $\pm$ 0.05 490.7/477
Mrk 876(a)9 177 $\pm$ 24 1.87 $\pm$ 0.11 326.9/320
PG 1626+55412 $\rm 145^{+22}_{-24}$ 2.09 $\pm$ 0.07 388.5/388


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