Table A2.

Best-fitting parameters of the photoionization absorption (xabs) and emission (pion) models applied on the continuum model for the time-average and flux-resolved spectra. The line width, σv, of them are linked together. Here the velocity, vLOS, are the absolute values of the line-of-sight velocity shown in SPEX, which has not been relativistically corrected yet. The uncertainties are estimated at 68 per cent confidence level.

DescriptionParameterAvgF1F2F3F4F5F6F7
xabsNH (1023 cm−2)|$0.26^{+0.09}_{-0.02}$||$0.18^{+0.05}_{-0.05}$||$0.80^{+0.05}_{-0.23}$||$0.6^{+0.2}_{-0.1}$||$1.0^{+0.4}_{-0.2}$||$1.2^{+0.4}_{-0.4}$||$1.2^{+0.3}_{-0.3}$||$3.2^{+1.1}_{-2.4}$|
log ξ (erg cm s−1)|$4.20^{+0.08}_{-0.01}$||$3.93^{+0.05}_{-0.06}$||$4.59^{+0.01}_{-0.11}$||$4.32^{+0.08}_{-0.08}$||$4.52^{+0.07}_{-0.08}$||$4.90^{+0.17}_{-0.17}$||$4.87^{+0.18}_{-0.15}$||$5.70^{+0.30}_{-0.27}$|
|vLOS| (km s−1)|$46594^{+577}_{-1806}$||$53197^{+1765}_{-1985}$||$44788^{+1395}_{-1364}$||$45827^{+1475}_{-1543}$||$45602^{+2250.64}_{-1466.45}$||$44094^{+1548}_{-1290}$||$40738^{+1563}_{-2110}$||$41832^{+3169}_{-2796}$|
σv (km s−1)|$4986^{+709}_{-276}$||$4630^{+973}_{-774}$||$4630^{+787}_{-981}$||$4535^{+1088}_{-622}$||$8373^{+1279}_{-1194}$||$4800^{+2767}_{-1529}$||$7077^{+1400}_{-1258}$|5000
pionNH (1021 cm−2)|$1.8^{+0.2}_{-0.2}$||$2.3^{+0.6}_{-0.5}$||$2.9^{+0.4}_{-0.4}$||$2.5^{+0.6}_{-0.5}$||$2.5^{+1.0}_{-0.5}$||$1.2^{+0.5}_{-0.2}$||$1.9^{+0.5}_{-0.4}$||$0.6^{+0.5}_{-0.3}$|
log ξ (erg cm s−1)|$2.68^{+0.02}_{-0.04}$||$2.69^{+0.07}_{-0.08}$||$2.75^{+0.06}_{-0.06}$||$2.64^{+0.07}_{-0.08}$||$2.54^{+0.08}_{-0.07}$||$2.44^{+0.13}_{-0.14}$||$2.59^{+0.05}_{-0.05}$||$2.35^{+0.20}_{-0.25}$|
|vLOS| (km s−1)|$7574^{+572}_{-437}$||$8457^{+760}_{-973}$||$6654^{+954}_{-913}$||$9269^{+726}_{-928}$||$8007^{+1418}_{-1055}$||$7117^{+1157}_{-1122}$||$9736^{+1001}_{-2369}$||$9088^{+1808}_{-2316}$|
C-statistic/dof2639/18002233/18201906/17331801/17301957/17431866/17751873/17571936/1781
DescriptionParameterAvgF1F2F3F4F5F6F7
xabsNH (1023 cm−2)|$0.26^{+0.09}_{-0.02}$||$0.18^{+0.05}_{-0.05}$||$0.80^{+0.05}_{-0.23}$||$0.6^{+0.2}_{-0.1}$||$1.0^{+0.4}_{-0.2}$||$1.2^{+0.4}_{-0.4}$||$1.2^{+0.3}_{-0.3}$||$3.2^{+1.1}_{-2.4}$|
log ξ (erg cm s−1)|$4.20^{+0.08}_{-0.01}$||$3.93^{+0.05}_{-0.06}$||$4.59^{+0.01}_{-0.11}$||$4.32^{+0.08}_{-0.08}$||$4.52^{+0.07}_{-0.08}$||$4.90^{+0.17}_{-0.17}$||$4.87^{+0.18}_{-0.15}$||$5.70^{+0.30}_{-0.27}$|
|vLOS| (km s−1)|$46594^{+577}_{-1806}$||$53197^{+1765}_{-1985}$||$44788^{+1395}_{-1364}$||$45827^{+1475}_{-1543}$||$45602^{+2250.64}_{-1466.45}$||$44094^{+1548}_{-1290}$||$40738^{+1563}_{-2110}$||$41832^{+3169}_{-2796}$|
σv (km s−1)|$4986^{+709}_{-276}$||$4630^{+973}_{-774}$||$4630^{+787}_{-981}$||$4535^{+1088}_{-622}$||$8373^{+1279}_{-1194}$||$4800^{+2767}_{-1529}$||$7077^{+1400}_{-1258}$|5000
pionNH (1021 cm−2)|$1.8^{+0.2}_{-0.2}$||$2.3^{+0.6}_{-0.5}$||$2.9^{+0.4}_{-0.4}$||$2.5^{+0.6}_{-0.5}$||$2.5^{+1.0}_{-0.5}$||$1.2^{+0.5}_{-0.2}$||$1.9^{+0.5}_{-0.4}$||$0.6^{+0.5}_{-0.3}$|
log ξ (erg cm s−1)|$2.68^{+0.02}_{-0.04}$||$2.69^{+0.07}_{-0.08}$||$2.75^{+0.06}_{-0.06}$||$2.64^{+0.07}_{-0.08}$||$2.54^{+0.08}_{-0.07}$||$2.44^{+0.13}_{-0.14}$||$2.59^{+0.05}_{-0.05}$||$2.35^{+0.20}_{-0.25}$|
|vLOS| (km s−1)|$7574^{+572}_{-437}$||$8457^{+760}_{-973}$||$6654^{+954}_{-913}$||$9269^{+726}_{-928}$||$8007^{+1418}_{-1055}$||$7117^{+1157}_{-1122}$||$9736^{+1001}_{-2369}$||$9088^{+1808}_{-2316}$|
C-statistic/dof2639/18002233/18201906/17331801/17301957/17431866/17751873/17571936/1781

Note. The parameter is pegged at this value.

Table A2.

Best-fitting parameters of the photoionization absorption (xabs) and emission (pion) models applied on the continuum model for the time-average and flux-resolved spectra. The line width, σv, of them are linked together. Here the velocity, vLOS, are the absolute values of the line-of-sight velocity shown in SPEX, which has not been relativistically corrected yet. The uncertainties are estimated at 68 per cent confidence level.

DescriptionParameterAvgF1F2F3F4F5F6F7
xabsNH (1023 cm−2)|$0.26^{+0.09}_{-0.02}$||$0.18^{+0.05}_{-0.05}$||$0.80^{+0.05}_{-0.23}$||$0.6^{+0.2}_{-0.1}$||$1.0^{+0.4}_{-0.2}$||$1.2^{+0.4}_{-0.4}$||$1.2^{+0.3}_{-0.3}$||$3.2^{+1.1}_{-2.4}$|
log ξ (erg cm s−1)|$4.20^{+0.08}_{-0.01}$||$3.93^{+0.05}_{-0.06}$||$4.59^{+0.01}_{-0.11}$||$4.32^{+0.08}_{-0.08}$||$4.52^{+0.07}_{-0.08}$||$4.90^{+0.17}_{-0.17}$||$4.87^{+0.18}_{-0.15}$||$5.70^{+0.30}_{-0.27}$|
|vLOS| (km s−1)|$46594^{+577}_{-1806}$||$53197^{+1765}_{-1985}$||$44788^{+1395}_{-1364}$||$45827^{+1475}_{-1543}$||$45602^{+2250.64}_{-1466.45}$||$44094^{+1548}_{-1290}$||$40738^{+1563}_{-2110}$||$41832^{+3169}_{-2796}$|
σv (km s−1)|$4986^{+709}_{-276}$||$4630^{+973}_{-774}$||$4630^{+787}_{-981}$||$4535^{+1088}_{-622}$||$8373^{+1279}_{-1194}$||$4800^{+2767}_{-1529}$||$7077^{+1400}_{-1258}$|5000
pionNH (1021 cm−2)|$1.8^{+0.2}_{-0.2}$||$2.3^{+0.6}_{-0.5}$||$2.9^{+0.4}_{-0.4}$||$2.5^{+0.6}_{-0.5}$||$2.5^{+1.0}_{-0.5}$||$1.2^{+0.5}_{-0.2}$||$1.9^{+0.5}_{-0.4}$||$0.6^{+0.5}_{-0.3}$|
log ξ (erg cm s−1)|$2.68^{+0.02}_{-0.04}$||$2.69^{+0.07}_{-0.08}$||$2.75^{+0.06}_{-0.06}$||$2.64^{+0.07}_{-0.08}$||$2.54^{+0.08}_{-0.07}$||$2.44^{+0.13}_{-0.14}$||$2.59^{+0.05}_{-0.05}$||$2.35^{+0.20}_{-0.25}$|
|vLOS| (km s−1)|$7574^{+572}_{-437}$||$8457^{+760}_{-973}$||$6654^{+954}_{-913}$||$9269^{+726}_{-928}$||$8007^{+1418}_{-1055}$||$7117^{+1157}_{-1122}$||$9736^{+1001}_{-2369}$||$9088^{+1808}_{-2316}$|
C-statistic/dof2639/18002233/18201906/17331801/17301957/17431866/17751873/17571936/1781
DescriptionParameterAvgF1F2F3F4F5F6F7
xabsNH (1023 cm−2)|$0.26^{+0.09}_{-0.02}$||$0.18^{+0.05}_{-0.05}$||$0.80^{+0.05}_{-0.23}$||$0.6^{+0.2}_{-0.1}$||$1.0^{+0.4}_{-0.2}$||$1.2^{+0.4}_{-0.4}$||$1.2^{+0.3}_{-0.3}$||$3.2^{+1.1}_{-2.4}$|
log ξ (erg cm s−1)|$4.20^{+0.08}_{-0.01}$||$3.93^{+0.05}_{-0.06}$||$4.59^{+0.01}_{-0.11}$||$4.32^{+0.08}_{-0.08}$||$4.52^{+0.07}_{-0.08}$||$4.90^{+0.17}_{-0.17}$||$4.87^{+0.18}_{-0.15}$||$5.70^{+0.30}_{-0.27}$|
|vLOS| (km s−1)|$46594^{+577}_{-1806}$||$53197^{+1765}_{-1985}$||$44788^{+1395}_{-1364}$||$45827^{+1475}_{-1543}$||$45602^{+2250.64}_{-1466.45}$||$44094^{+1548}_{-1290}$||$40738^{+1563}_{-2110}$||$41832^{+3169}_{-2796}$|
σv (km s−1)|$4986^{+709}_{-276}$||$4630^{+973}_{-774}$||$4630^{+787}_{-981}$||$4535^{+1088}_{-622}$||$8373^{+1279}_{-1194}$||$4800^{+2767}_{-1529}$||$7077^{+1400}_{-1258}$|5000
pionNH (1021 cm−2)|$1.8^{+0.2}_{-0.2}$||$2.3^{+0.6}_{-0.5}$||$2.9^{+0.4}_{-0.4}$||$2.5^{+0.6}_{-0.5}$||$2.5^{+1.0}_{-0.5}$||$1.2^{+0.5}_{-0.2}$||$1.9^{+0.5}_{-0.4}$||$0.6^{+0.5}_{-0.3}$|
log ξ (erg cm s−1)|$2.68^{+0.02}_{-0.04}$||$2.69^{+0.07}_{-0.08}$||$2.75^{+0.06}_{-0.06}$||$2.64^{+0.07}_{-0.08}$||$2.54^{+0.08}_{-0.07}$||$2.44^{+0.13}_{-0.14}$||$2.59^{+0.05}_{-0.05}$||$2.35^{+0.20}_{-0.25}$|
|vLOS| (km s−1)|$7574^{+572}_{-437}$||$8457^{+760}_{-973}$||$6654^{+954}_{-913}$||$9269^{+726}_{-928}$||$8007^{+1418}_{-1055}$||$7117^{+1157}_{-1122}$||$9736^{+1001}_{-2369}$||$9088^{+1808}_{-2316}$|
C-statistic/dof2639/18002233/18201906/17331801/17301957/17431866/17751873/17571936/1781

Note. The parameter is pegged at this value.

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