Table 10: Spectral fitting results. VII: best fit model. A: bb; B: diskbb; C: brems; D: power law; E: double bb; F: absori; G: double absori + bb; H: partial-covering (cold)+raymond-smith; I: partial-covering(warm)+emission line; J: absori+bb; PL: simple power law. Models with * include an additional cold absorption component. All but one (i.e. model PL) models also include a power law component. For the results concerning the Fe K$\alpha $ line see Paper II.
PG name Model $\Gamma$ $kT/\Gamma_{\rm soft}$ kT $\xi$/($N_{\rm H}$) Edge/$\tau$ $\chi^2$($\nu$) Fe K$\alpha $
      (keV) (keV) (keV)/1022 cm-2 (keV)    
0007+106 A $\rm 1.71^{+0.04}_{-0.04}$ $\rm0.16^{+0.01}_{-0.01}$ - - - 312(302) Y
0050+124 E* $\rm 2.31^{+0.03}_{-0.03}$ $\rm0.084^{+0.008}_{-0.008}$ $\rm0.19^{+0.03}_{-0.02}$ $\rm0.09^{+0.02}_{-0.02}$ $\rm0.647^{+0.009}_{-0.009}/0.26^{+0.06}_{-0.06}$ 523(383) Y
0157+001 A $\rm 2.24^{+0.06}_{-0.07}$ $\rm0.125^{+0.012}_{-0.014}$ - - - 149(166) N
0804+761 D $\rm 1.3^{+0.7}_{-0.7}$ $\rm 2.5^{+0.4}_{-0.1}$ - - - 287(262) Y
0844+349 E $\rm 1.96^{+0.09}_{-0.06}$ $\rm0.112^{+0.008}_{-0.004}$ $\rm0.33^{+0.03}_{-0.03}$ - - 162(162) N
0947+396 C $\rm 1.83^{+0.07}_{-0.05}$ $\rm0.50^{+0.05}_{-0.04}$ - - $\rm0.79^{+0.04}_{-0.03}/0.18^{+0.04}_{-0.04}$ 218(259) Y
0953+414 E $\rm 1.97^{+0.04}_{-0.04}$ $\rm0.119^{+0.009}_{-0.009}$ $\rm0.25^{+0.02}_{-0.02}$ - $\rm0.73^{+0.03}_{-0.03}/0.18^{+0.06}_{-0.09}$ 308(284) N
1001+054 F $\rm 2.0^{+0.2}_{-0.1}$ - - $\rm 542 ^{+97}_{-147}/19.2^{+11.9}_{-7.3}$ - 16(8) N
1048+342 E $\rm 1.74^{+0.08}_{-0.08}$ $\rm0.115^{+0.008}_{-0.010}$ $\rm0.27^{+0.04}_{-0.02}$ - - 243(269) Y
1100+772 E $\rm 1.57^{+0.07}_{-0.07}$ $\rm0.133^{+0.004}_{-0.007}$ $\rm0.4^{+0.03}_{-0.03}$ - - 339(342) Y
1114+445 G $\rm 1.85^{+0.04}_{-0.03}$ $\rm0.207^{+0.09}_{-0.09}$ - $\rm 89 ^{+37}_{-30}/1.5^{+0.4}_{-0.3}$ $\rm 4.0^{+0.5}_{-0.5}/1.53^{+0.12}_{-0.07}$a 315(360) Y
1115+080 PL* $\rm 1.85^{+0.05}_{-0.05}$ - - $\rm0.33^{+0.08}_{-0.07}$ $\rm 7.1^{+0.3}_{-0.4}/0.28^{+0.13}_{-0.12}$ 214(217) N
            $\rm 9.5^{+0.3}_{-0.3}/0.31^{+0.17}_{-0.15}$ 204(215)  
1115+407 E $\rm 2.18^{+0.08}_{-0.08}$ $\rm0.097^{+0.006}_{-0.006}$ $\rm0.238^{+0.003}_{-0.003}$ - - 228(230) Y
1116+215 C $\rm 2.20^{+0.06}_{-0.07}$ $\rm0.32^{+0.04}_{-0.04}$ - - $\rm0.75^{+0.05}_{-0.06}/0.10^{+0.07}_{-0.06}$ 197(228) Y
1202+281 C $\rm 1.68^{+0.05}_{-0.05}$ $\rm0.49^{+0.05}_{-0.05}$ - - $\rm0.74^{+0.03}_{-0.03}/0.20^{+0.06}_{-0.06}$ 306(319) N
1206+459 PL $\rm 1.74^{+0.09}_{-0.09}$ - - - - 40(42) N
1211+143 E $\rm 1.61^{+0.05}_{-0.03}$ $\rm0.113^{+0.002}_{-0.004}$ $\rm0.24^{+0.02}_{-0.03}$ - $\rm0.775^{+0.11}_{-0.05}/0.39^{+0.04}_{-0.04}$ 402(392) Y
            $\rm0.967^{+0.010}_{-0.009}/0.39^{+0.04}_{-0.06}$    
            $\rm 7.25^{+0.14}_{-0.09}/0.66^{+0.12}_{-0.07}$    
1216+069 E $\rm 1.67^{+0.06}_{-0.09}$ $\rm0.123^{+0.07}_{-0.09}$ $\rm0.349^{+0.05}_{-0.05}$ - - 164(200) N
1226+023 E $\rm 1.60^{+0.01}_{-0.01}$ $\rm0.10^{+0.02}_{-0.02}$ $\rm0.24^{+0.01}_{-0.01}$ - $\rm 7.4^{+0.1}_{-0.2}/0.10^{+0.01}_{-0.03}$ 320(258) N
1244+026 A $\rm 2.48^{+0.03}_{-0.03}$ $\rm0.16^{+0.01}_{-0.01}$ - - - 125(110) N
1307+085 A $\rm 1.50^{+0.04}_{-0.04}$ $\rm0.13^{+0.01}_{-0.01}$ - - $\rm0.74^{+0.02}_{-0.02}/0.54^{+0.10}_{-0.14}$ 232(210) N
1309+355 A $\rm 1.81^{+0.04}_{-0.04}$ $\rm0.103^{+0.011}_{-0.007}$ - - $\rm0.75^{+0.03}_{-0.03}/0.4^{+0.2}_{-0.1}$ 225(214) Y
1322+659 C $\rm 2.25^{+0.06}_{-0.08}$ $\rm0.29^{+0.01}_{-0.02}$ - - - 235(212) Y
1352+183 E $\rm 1.84^{+0.14}_{-0.10}$ $\rm0.112^{+0.012}_{-0.011}$ $\rm0.26^{+0.03}_{-0.03}$ - $\rm0.69^{+0.03}_{-0.04}/0.21^{+0.09}_{-0.11}$ 247(240) Y
1402+261 C $\rm 2.15^{+0.08}_{-0.07}$ $\rm0.37^{+0.03}_{-0.03}$ - - $\rm0.75^{+0.04}_{-0.04}/0.17^{+0.07}_{-0.06}$ 204(213) Y
1404+226 J $\rm 2.3^{+0.4}_{-0.4}$ $\rm0.114^{+0.002}_{-0.003}$ - $\rm 44^{+123}_{-26}/1.4^{+0.6}_{-0.3}$ - 60(75) N
1407+265 A $\rm 2.21^{+0.03}_{-0.03}$ $\rm0.20^{+0.03}_{-0.03}$ - - - 223(244) N
1411+442 H $\rm 2.3^{+0.2}_{-0.2}$ $\equiv\Gamma$ $\rm0.15^{+0.03}_{-0.03}$ $\rm 23.2^{+3.8}_{-3.8}$c - 82(102) Y
1415+451 E $\rm 2.00^{+0.07}_{-0.10}$ $\rm0.099^{+0.006}_{-0.006}$ $\rm0.24^{+0.03}_{-0.03}$ - - 169(126) Y
1427+480 C $\rm 1.93^{+0.06}_{-0.03}$ $\rm0.44^{+0.04}_{-0.04}$ - - $\rm0.76^{+0.03}_{-0.04}/0.12^{+0.05}_{-0.04}$ 251(277) Y
1440+356 D $\rm 1.2^{+0.4}_{-0.2}$ $\rm 3.14^{+0.2}_{-0.08}$ - - - 191(158) N
1444+407 D $\rm 1.8^{+0.3}_{-0.3}$ $\rm 3.3^{+0.2}_{-0.3}$ - - - 196(166) N
1501+106 E $\rm 1.84^{+0.02}_{-0.02}$ $\rm0.0937^{+0.0014}_{-0.002}$ $\rm0.235^{+0.005}_{-0.007}$ - - 240(221) N
1512+370 D $\rm 1.51^{+0.09}_{-0.09}$ $\rm 2.71^{+0.22}_{-0.15}$ - - - 226(253) Y
1613+658 A $\rm 1.80^{+0.07}_{-0.03}$ $\rm0.13^{+0.01}_{-0.01}$ - - $\rm0.73^{+0.02}_{-0.02}/0.5^{+0.1}_{-0.2}$ 148(180) N
1626+554 D $\rm 1.9^{+0.1}_{-0.4}$ $\rm 3.1^{+0.7}_{-0.4}$ - - - 266(268) N
1630+377 D $\rm 1.9^{+0.3}_{-0.3}$ $\rm 3.4^{+2.4}_{-1.1}$ - - - 44(57) Y
1634+706 C $\rm 1.95^{+0.11}_{-0.08}$ $\rm 1.1^{+0.2}_{-0.2}$ - - - 203(208) N
2214+139 I $\rm 1.88^{+0.04}_{-0.04}$ $\equiv\Gamma$ $\rm0.57^{+0.02}_{-0.01}$b $\rm 89^{+14}_{-12}/8.9^{+0.5}_{-0.5}$ $\rm 6^{+3}_{-1}/1.7^{+0.2}_{-0.4}$a 335(358) Y
2302+029 C $\rm 2.03^{+0.06}_{-0.11}$ $\rm0.37^{+0.13}_{-0.11}$ - - - 58(66) N
a Values of $\xi$ and $N_{\rm H}$ of the second warm absorber component in erg/cm2/s and 1022 cm-2, respectively; b energy (in keV) of the emission line (see text for details); c value of $N_{\rm H} \times 10^{22}$ cm-2.

Source LaTeX | All tables | In the text

Article Contents
1 Introduction
2 XMM-Newton observations
3 Analysis of the spectra
4 Discussion
5 Conclusions
References
Online Material
List of tables
List of figures