Table 3: XMM- Newton EPIC-PN spectral fitting results using the photoionized gas model described in the text. Fluxes are given in units of 10^-13 erg cm^-2 s^-1, luminosities in units of 10⁴³ erg s^-1; both are corrected for absorption. ^* denotes a fixed parameter.
1 APEC 2 APEC

Apec(1)

kT [keV] $\rm0.66^{+0.07}_{-0.04}$ $\rm0.76^{+0.08}_{-0.07}$

$f~_{0.3 - 10\: {\rm keV}}$ $0.62\pm0.07$ $0.52\pm0.11$

Apec(2)

kT [keV] - $\rm0.26^{+0.08}_{-0.03}$

$f~_{0.3 - 10\: {\rm keV}}$ - $\rm0.23^{+0.11}_{-0.10}$

Power-law(1)

$N_{\rm H}$ [10²² cm^-2] $\rm 68^{+17}_{-15}$ $\rm 65^{+15}_{-12}$

$\Gamma$ 1.9^* 1.9^*

$f~_{0.3 - 10\: {\rm keV}}$ $\rm 41_{-12}^{+21}$ $\rm 39_{-11}^{+20}$

Power-law(2)

$N{\rm _{H}}$ [10²⁰ cm^-2] 7^* 7^*

$\Gamma$ 1.9^* 1.9^*

$f~_{0.3 - 10\: {\rm keV}}$ $1.7\pm0.2$ $1.5\pm0.2$

Fe K $\alpha$

E [keV] 6.4^* 6.4^*

EW [eV] $\rm 186_{-125}^{+165}$ $\rm 185_{-122}^{+159}$

$f~_{0.3 - 10\: {\rm keV}}$ $\rm0.50^{+0.44}_{-0.34}$ $\rm0.47^{+0.40}_{-0.31}$

Fe XXV

E [keV] 6.7^* 6.7^*

EW [eV] $\rm 121_{-102}^{+110}$ $\rm 124_{-103}^{+110}$

$f~_{0.3 - 10\: {\rm keV}}$ $\rm0.34^{+0.31}_{-0.29}$ $\rm0.33^{+0.29}_{-0.27}$

Total

$f~_{0.3 - 10\: {\rm keV}}$ 44.5 42.1

$L~_{0.3 - 10\: {\rm keV}}$ 1.47 1.39

$\chi^2/$ d.o.f. 84.9/80 64.0/78

**Table 3:** XMM- *Newton* EPIC-PN spectral fitting results using the photoionized gas model described in the text. Fluxes are given in units of 10^-13 erg cm^-2 s^-1, luminosities in units of 10⁴³ erg s^-1; both are corrected for absorption. ^* denotes a fixed parameter.
	1 APEC	2 APEC
Apec(1)
kT [keV]	$\rm0.66^{+0.07}_{-0.04}$	$\rm0.76^{+0.08}_{-0.07}$
$f~_{0.3 - 10\: {\rm keV}}$	$0.62\pm0.07$	$0.52\pm0.11$
Apec(2)
kT [keV]	-	$\rm0.26^{+0.08}_{-0.03}$
$f~_{0.3 - 10\: {\rm keV}}$	-	$\rm0.23^{+0.11}_{-0.10}$
Power-law(1)
$N_{\rm H}$ [10²² cm^-2]	$\rm 68^{+17}_{-15}$	$\rm 65^{+15}_{-12}$
$\Gamma$	1.9^*	1.9^*
$f~_{0.3 - 10\: {\rm keV}}$	$\rm 41_{-12}^{+21}$	$\rm 39_{-11}^{+20}$
Power-law(2)
$N{\rm _{H}}$ [10²⁰ cm^-2]	7^*	7^*
$\Gamma$	1.9^*	1.9^*
$f~_{0.3 - 10\: {\rm keV}}$	$1.7\pm0.2$	$1.5\pm0.2$
Fe K $\alpha$
E [keV]	6.4^*	6.4^*
EW [eV]	$\rm 186_{-125}^{+165}$	$\rm 185_{-122}^{+159}$
$f~_{0.3 - 10\: {\rm keV}}$	$\rm0.50^{+0.44}_{-0.34}$	$\rm0.47^{+0.40}_{-0.31}$
Fe XXV
E [keV]	6.7^*	6.7^*
EW [eV]	$\rm 121_{-102}^{+110}$	$\rm 124_{-103}^{+110}$
$f~_{0.3 - 10\: {\rm keV}}$	$\rm0.34^{+0.31}_{-0.29}$	$\rm0.33^{+0.29}_{-0.27}$
Total
$f~_{0.3 - 10\: {\rm keV}}$	44.5	42.1
$L~_{0.3 - 10\: {\rm keV}}$	1.47	1.39
$\chi^2/$ d.o.f.	84.9/80	64.0/78

Source LaTeX | All tables | In the text

	1 Introduction
	2 Observations and data reduction
	3 Spectral analysis
	4 Comparison with Chandra
	5 Discussion
	6 Conclusions
	Appendix A: The unabsorbed Seyfert 2 Mrk 273x
	References