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Table 2.

Results of the fit to the spectra of NGC 3227.

Parameter Epoch A Epoch B Epoch C Epoch D Epoch E Epoch F Epoch G Epoch H Epoch I
Model I : const*TBabs*zTBabs(zpo + zgauss)

Γ 1.56 1.55 1.61 1.63 1.66 1.63 1.61 1.64 1.48
NH(zTBabs) 2.91 4.66 4.57
E 6.35 6.38 6.33 6.32 6.30 6.34 6.23 6.28 6.38
EW 149 188 142 129 86 115 115 123 269
Norm 71 58 73 90 101 92 122 76 17
χ2/d.o.f. 930/826 752/706 834/704 909/777 815/790 684/717 1081/935 600/595 257/247
CFPMA/FPMB 1.04 1.02 1.01 1.01 1.02 1.00 0.99 1.04 1.06

Model II : const*TBabs*zTBabs(pexrav + zgauss)

Γ 1.68 1.64 1.77 1.83 1.88 1.82 1.92 1.85 1.70
NH(zTBabs) 6.43 7.71 8.52
Ecut 212 163 > 254 > 1147 > 411 > 406 > 571 > 775 > 126
R 0.52 0.48 0.53 0.55 0.73 0.55 0.83 0.45 0.38
E 6.35 6.38 6.33 6.32 6.31 6.34 6.23 6.28 6.38
EW 137 177 129 116 74 102 85 102 231
Norm 84 66 91 119 139 120 207 112 25
χ2/d.o.f. 856/824 711/704 784/702 831/775 714/788 625/715 920/933 577/593 253/245
CFPMA/FPMB 1.04 1.02 1.01 1.01 1.02 1.00 0.99 1.04 1.06

Model III : const*TBabs*zTBabs(xillver)

Γ 1.69 1.69 1.77 1.83 1.80 1.79 1.77 1.87 1.91
NH(zTBabs) 4.73 8.58 12.12
Ecut 127 92 204 > 439 378 326 248 > 510 > 198
R 0.86 1.09 0.85 0.76 0.61 0.71 0.68 0.64 1.36
Norm 1.98 1.46 2.01 2.98 2.97 2.75 3.73 2.72 0.68
χ2/d.o.f. 868/826 728/706 785/704 837/777 735/790 627/717 976/935 579/595 260/247
CFPMA/FPMB 1.04 1.02 1.01 1.01 1.02 1.00 0.99 1.04 1.06

Model IV : const*TBabs*zTBabs(xillverCP)

Γ 1.78 1.80 1.83 1.84 1.83 1.83 1.82 1.87 1.91
NH(zTBabs) 4.97 8.17 12.21
kTe 33 28 56 > 80 > 45 > 47 50 > 85 > 36
R 0.79+0.11−0.11 0.96+0.18−0.10 0.83 0.78 0.62 0.71 0.67 0.65 1.28
Norm 1.94 1.52 1.89 2.56 2.55 2.50 3.32 2.24 0.66
χ2/d.o.f. 881/826 746/706 790/704 838/777 733/790 629/717 970/935 581/595 261/247
CFPMA/FPMB 1.04 1.02 1.01 1.01 1.02 1.00 0.99 1.04 1.06
Flux 1.04 0.86 0.94 1.11 1.15 1.13 1.55 0.88 0.27

Notes. Models are Model I: const*TBabs*zTBabs(zpo + zgauss), Model II: const*TBabs*zTBabs(pexrav + zgauss), Model III: const*TBabs*zTBabs(xillver), and Model IV: const*TBabs*zTBabs(xillverCP). The zTBabs component is added with all the models to fit the epoch G, H, and I spectra. The fluxes are in units of 10−10 erg cm−2 s−1 in the 4–60 keV band except in epoch I, where the flux was calculated in the 4–50 keV band. The energy (E) of the FeKα line, the equivalent width (EW) of the line, Ecut, and kTe are expressed in units of keV, model normalization is in units of 10−4 photons keV−1 cm−2 s−1, and NH(zTBabs) is the host galaxy hydrogen column density in units of 1022 atoms cm−2. CFPMA/FPMB is the cross-calibration constant. The width of the FeKα line was fixed to 0.1 keV during the fitting.

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