Table 2. Open in new tab The strongest...

Transition	ΔC-stat	Rest-frame	Best-fitting^a	Norm	FWHM
Absorption
N vii	69	0.500	\|$0.601^{+0.004}_{-0.004}$\|	\|$-1.7^{+0.2}_{-0.3}$\|	\|$0.047^{+0.006}_{-0.007}$\|
O viii	110	0.653	\|$0.767^{+0.003}_{-0.003}$\|	\|$-1.7^{+0.2}_{-0.2}$\|	\|$0.093^{+0.008}_{-0.007}$\|
Fe xvii	65	0.826	\|$0.996^{+0.003}_{-0.003}$\|	\|$-1.0^{+0.2}_{-0.2}$\|	\|$0.062^{+0.009}_{-0.008}$\|
Ne x	122	1.022	\|$1.216^{+0.009}_{-0.010}$\|	\|$-1.7^{+0.4}_{-0.2}$\|	\|$0.28^{+0.02}_{-0.02}$\|
Fe xxv/xxvi	106	6.699/6.973	\|$7.70^{+0.02}_{-0.02}$\|	\|$-0.12^{+0.02}_{-0.01}$\|	\|$0.81^{+0.04}_{-0.08}$\|
Emission
N vii	251	0.500	\|$0.508^{+0.001}_{-0.002}$\|	\|$3.8^{+0.5}_{-0.3}$\|	\|$0.046^{+0.005}_{-0.003}$\|
O viii	202	0.653	\|$0.669^{+0.001}_{-0.001}$\|	\|$1.1^{+0.1}_{-0.1}$\|	\|$0.021^{+0.003}_{-0.002}$\|
Fe xvii	79	0.826	\|$0.884^{+0.003}_{-0.004}$\|	\|$1.1^{+0.2}_{-0.2}$\|	\|$0.086^{+0.008}_{-0.011}$\|
Ne x	49	1.022	\|$1.075^{+0.003}_{-0.007}$\|	\|$0.58^{+0.10}_{-0.05}$\|	\|$0.066^{+0.008}_{-0.006}$\|
Fe xxv/xxvi	121	6.699/6.973	\|$6.86^{+0.02}_{-0.02}$\|	\|$0.08^{+0.02}_{-0.01}$\|	\|$0.66^{+0.07}_{-0.05}$\|

Transition

ΔC-stat

Rest-frame

Best-fitting^a

Norm

FWHM

energy (keV)

(10⁵⁰ ph s⁻¹)

(keV)

Absorption

N vii

0.500

|$0.601^{+0.004}_{-0.004}$|

|$-1.7^{+0.2}_{-0.3}$|

|$0.047^{+0.006}_{-0.007}$|

O viii

110

0.653

|$0.767^{+0.003}_{-0.003}$|

|$-1.7^{+0.2}_{-0.2}$|

|$0.093^{+0.008}_{-0.007}$|

Fe xvii

0.826

|$0.996^{+0.003}_{-0.003}$|

|$-1.0^{+0.2}_{-0.2}$|

|$0.062^{+0.009}_{-0.008}$|

Ne x

122

1.022

|$1.216^{+0.009}_{-0.010}$|

|$-1.7^{+0.4}_{-0.2}$|

|$0.28^{+0.02}_{-0.02}$|

Fe xxv/xxvi

106

6.699/6.973

|$7.70^{+0.02}_{-0.02}$|

|$-0.12^{+0.02}_{-0.01}$|

|$0.81^{+0.04}_{-0.08}$|

Emission

N vii

251

0.500

|$0.508^{+0.001}_{-0.002}$|

|$3.8^{+0.5}_{-0.3}$|

|$0.046^{+0.005}_{-0.003}$|

O viii

202

0.653

|$0.669^{+0.001}_{-0.001}$|

|$1.1^{+0.1}_{-0.1}$|

|$0.021^{+0.003}_{-0.002}$|

Fe xvii

0.826

|$0.884^{+0.003}_{-0.004}$|

|$1.1^{+0.2}_{-0.2}$|

|$0.086^{+0.008}_{-0.011}$|

Ne x

1.022

|$1.075^{+0.003}_{-0.007}$|

|$0.58^{+0.10}_{-0.05}$|

|$0.066^{+0.008}_{-0.006}$|

Fe xxv/xxvi

121

6.699/6.973

|$6.86^{+0.02}_{-0.02}$|

|$0.08^{+0.02}_{-0.01}$|

|$0.66^{+0.07}_{-0.05}$|

Transition	ΔC-stat	Rest-frame	Best-fitting^a	Norm	FWHM
Absorption
N vii	69	0.500	\|$0.601^{+0.004}_{-0.004}$\|	\|$-1.7^{+0.2}_{-0.3}$\|	\|$0.047^{+0.006}_{-0.007}$\|
O viii	110	0.653	\|$0.767^{+0.003}_{-0.003}$\|	\|$-1.7^{+0.2}_{-0.2}$\|	\|$0.093^{+0.008}_{-0.007}$\|
Fe xvii	65	0.826	\|$0.996^{+0.003}_{-0.003}$\|	\|$-1.0^{+0.2}_{-0.2}$\|	\|$0.062^{+0.009}_{-0.008}$\|
Ne x	122	1.022	\|$1.216^{+0.009}_{-0.010}$\|	\|$-1.7^{+0.4}_{-0.2}$\|	\|$0.28^{+0.02}_{-0.02}$\|
Fe xxv/xxvi	106	6.699/6.973	\|$7.70^{+0.02}_{-0.02}$\|	\|$-0.12^{+0.02}_{-0.01}$\|	\|$0.81^{+0.04}_{-0.08}$\|
Emission
N vii	251	0.500	\|$0.508^{+0.001}_{-0.002}$\|	\|$3.8^{+0.5}_{-0.3}$\|	\|$0.046^{+0.005}_{-0.003}$\|
O viii	202	0.653	\|$0.669^{+0.001}_{-0.001}$\|	\|$1.1^{+0.1}_{-0.1}$\|	\|$0.021^{+0.003}_{-0.002}$\|
Fe xvii	79	0.826	\|$0.884^{+0.003}_{-0.004}$\|	\|$1.1^{+0.2}_{-0.2}$\|	\|$0.086^{+0.008}_{-0.011}$\|
Ne x	49	1.022	\|$1.075^{+0.003}_{-0.007}$\|	\|$0.58^{+0.10}_{-0.05}$\|	\|$0.066^{+0.008}_{-0.006}$\|
Fe xxv/xxvi	121	6.699/6.973	\|$6.86^{+0.02}_{-0.02}$\|	\|$0.08^{+0.02}_{-0.01}$\|	\|$0.66^{+0.07}_{-0.05}$\|

Table 2.

Open in new tab

The strongest transition residuals fitted with a Gaussian.

Transition	ΔC-stat	Rest-frame	Best-fitting^a	Norm	FWHM
		energy (keV)	energy (keV)	(10⁵⁰ ph s⁻¹)	(keV)
Absorption
N vii	69	0.500	\|$0.601^{+0.004}_{-0.004}$\|	\|$-1.7^{+0.2}_{-0.3}$\|	\|$0.047^{+0.006}_{-0.007}$\|
O viii	110	0.653	\|$0.767^{+0.003}_{-0.003}$\|	\|$-1.7^{+0.2}_{-0.2}$\|	\|$0.093^{+0.008}_{-0.007}$\|
Fe xvii	65	0.826	\|$0.996^{+0.003}_{-0.003}$\|	\|$-1.0^{+0.2}_{-0.2}$\|	\|$0.062^{+0.009}_{-0.008}$\|
Ne x	122	1.022	\|$1.216^{+0.009}_{-0.010}$\|	\|$-1.7^{+0.4}_{-0.2}$\|	\|$0.28^{+0.02}_{-0.02}$\|
Fe xxv/xxvi	106	6.699/6.973	\|$7.70^{+0.02}_{-0.02}$\|	\|$-0.12^{+0.02}_{-0.01}$\|	\|$0.81^{+0.04}_{-0.08}$\|
Emission
N vii	251	0.500	\|$0.508^{+0.001}_{-0.002}$\|	\|$3.8^{+0.5}_{-0.3}$\|	\|$0.046^{+0.005}_{-0.003}$\|
O viii	202	0.653	\|$0.669^{+0.001}_{-0.001}$\|	\|$1.1^{+0.1}_{-0.1}$\|	\|$0.021^{+0.003}_{-0.002}$\|
Fe xvii	79	0.826	\|$0.884^{+0.003}_{-0.004}$\|	\|$1.1^{+0.2}_{-0.2}$\|	\|$0.086^{+0.008}_{-0.011}$\|
Ne x	49	1.022	\|$1.075^{+0.003}_{-0.007}$\|	\|$0.58^{+0.10}_{-0.05}$\|	\|$0.066^{+0.008}_{-0.006}$\|
Fe xxv/xxvi	121	6.699/6.973	\|$6.86^{+0.02}_{-0.02}$\|	\|$0.08^{+0.02}_{-0.01}$\|	\|$0.66^{+0.07}_{-0.05}$\|

Transition	ΔC-stat	Rest-frame	Best-fitting^a	Norm	FWHM
		energy (keV)	energy (keV)	(10⁵⁰ ph s⁻¹)	(keV)
Absorption
N vii	69	0.500	\|$0.601^{+0.004}_{-0.004}$\|	\|$-1.7^{+0.2}_{-0.3}$\|	\|$0.047^{+0.006}_{-0.007}$\|
O viii	110	0.653	\|$0.767^{+0.003}_{-0.003}$\|	\|$-1.7^{+0.2}_{-0.2}$\|	\|$0.093^{+0.008}_{-0.007}$\|
Fe xvii	65	0.826	\|$0.996^{+0.003}_{-0.003}$\|	\|$-1.0^{+0.2}_{-0.2}$\|	\|$0.062^{+0.009}_{-0.008}$\|
Ne x	122	1.022	\|$1.216^{+0.009}_{-0.010}$\|	\|$-1.7^{+0.4}_{-0.2}$\|	\|$0.28^{+0.02}_{-0.02}$\|
Fe xxv/xxvi	106	6.699/6.973	\|$7.70^{+0.02}_{-0.02}$\|	\|$-0.12^{+0.02}_{-0.01}$\|	\|$0.81^{+0.04}_{-0.08}$\|
Emission
N vii	251	0.500	\|$0.508^{+0.001}_{-0.002}$\|	\|$3.8^{+0.5}_{-0.3}$\|	\|$0.046^{+0.005}_{-0.003}$\|
O viii	202	0.653	\|$0.669^{+0.001}_{-0.001}$\|	\|$1.1^{+0.1}_{-0.1}$\|	\|$0.021^{+0.003}_{-0.002}$\|
Fe xvii	79	0.826	\|$0.884^{+0.003}_{-0.004}$\|	\|$1.1^{+0.2}_{-0.2}$\|	\|$0.086^{+0.008}_{-0.011}$\|
Ne x	49	1.022	\|$1.075^{+0.003}_{-0.007}$\|	\|$0.58^{+0.10}_{-0.05}$\|	\|$0.066^{+0.008}_{-0.006}$\|
Fe xxv/xxvi	121	6.699/6.973	\|$6.86^{+0.02}_{-0.02}$\|	\|$0.08^{+0.02}_{-0.01}$\|	\|$0.66^{+0.07}_{-0.05}$\|

The best-fitting energy of the Gaussian is in the AGN rest frame.

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