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Table 2.

Best-fit parameters of the ASCA spectra of NGC 7469 in the 0.45–10 keV range using the following five models: phabs*power, phabs*bbody, phabs*(bbody+power), phabs*bmc, and phabs*(bmc+Gaussian).

Model Parameter 71028000 71028010 71028030 15030000 18931126
phabs NH ( × 1021 cm−2) 2.7 ± 0.5 2.5 ± 0.9 1.8 ± 0.09 2.6 ± 0.2 2.9 ± 0.6
Power law Γpow 2.34 ± 0.02 2.29 ± 0.02 2.28 ± 0.03 2.31 ± 0.02 2.21 ± 0.04
Npow†† 0.019 ± 0.003 0.019 ± 0.001 0.015 ± 0.001 0.036 ± 0.001 0.017 ± 0.001

χ2 (d.o.f.) 2.17 (214) 2.55 (335) 1.85 (183) 1.56 (129) 0.92 (161)

phabs NH ( × 1021 cm−2) 3.7 ± 0.2 3.5 ± 0.3 4.7 ± 0.5 5.8 ± 0.3 2.9 ± 0.08
Blackbody TBB (keV) 0.54 ± 0.01 0.36 ± 0.01 0.95 ± 0.01 0.89 ± 0.01 0.26 ± 0.01
NBB†† 5.8 ± 0.4 4.1 ± 0.1 12.3 ± 0.4 5.7 ± 0.2 27.9 ± 0.7

χ2 (d.o.f.) 8.61 (214) 14.1 (335) 2.63 (183) 4.08 (129) 15.76 (161)

phabs NH ( × 1021 cm−2) 2.7 ± 0.3 2.7 ± 0.2 2.7 ± 0.6 3.2 ± 0.4 3.0 ± 0.1
Blackbody TBB (keV) 1.8 ± 0.1 1.87 ± 0.07 2.1 ± 0.2 1.72 ± 0.09 1.8 ± 0.2
NBB†† 3.3 ± 0.4 3.4 ± 0.3 2.8 ± 0.4 3.5 ± 0.4 3.0 ± 0.7
Power law Γpow 3.16 ± 0.07 3.07 ± 0.05 2.98 ± 0.08 3.02 ± 0.07 2.9 ± 0.1
Npow†† 0.03 ± 0.06 0.024 ± 0.04 0.019 ± 0.001 0.04 ± 0.01 0.02 ± 0.01

χ2 (d.o.f.) 1.12 (212) 1.11 (333) 1.01 (181) 0.96 (127) 0.62 (159)

phabs NH ( × 1021 cm−2) 3.5 ± 0.6 3.1 ± 0.6 2.9 ± 0.1 2.8 ± 0.3 3.0 ± 0.1
bmc Γbmc 1.8 ± 0.1 1.86 ± 0.04 1.74 ± 0.07 1.81 ± 0.06 1.64 ± 0.09
Ts (eV) 140 ± 30 160 ± 20 200 ± 40 220 ± 30 210 ± 20
log A 0.33 ± 0.07 0.36 ± 0.02 0.34 ± 0.05 0.32 ± 0.02 0.36 ± 0.05
Nbmc†† 7.56 ± 0.04 7.2 ± 0.1 6.1 ± 0.1 6.9 ± 0.1 6.58 ± 0.05

phabs*bmc χ2 (d.o.f.) 1.08 (212) 1.19 (333) 1.09 (181) 1.12 (227) 0.89 (159)

Gaussian Eline (keV) 6.4 ± 0.1 6.3 ± 0.1 6.4 ± 0.2 6.41 ± 0.03 6.38 ± 0.09
σline (eV) 200 ± 10 150 ± 60 170 ± 90 110 ± 30 160 ± 30
Nline 8.9 ± 0.3 3.7 ± 0.5 5.3 ± 0.1 1.6 ± 0.2 9.4 ± 0.5
phabs*(bmc+Gaussian) χ2 (d.o.f.) 1.01 (209) 1.12 (330) 1.08 (178) 1.07 (224) 0.95 (156)

Notes. Errors are given at the 90% confidence level.

(††)

Normalization parameters of blackbody and bmc components are in units of erg s−1 kpc−2, where is soft photon luminosity in units of 1034 erg s−1, d10 is the distance to the source in units of 10 kpc, while power–law and Gaussian components are in units of keV−1 cm−2 s−1 at 1 keV and 10−5 × total photons cm−2 s−1 at 1 keV, respectively. TBB and Ts are the temperatures of the blackbody and seed photon components, respectively (in keV and eV). Γpow and Γbmc are the indices of the power law and bmc, respectively.

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