Table 3.
Spectral fit results for the phenomenological model [(partcov*xstar500)*(xstar5000*pow + zgauss1 + zgauss2)].
2004 | 2008A | 2008B | 2009 | 2014A | 2014B | 2014C | 2015 | |
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Power law emission: pow | ||||||||
Γ |
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N1 keV/10−4 |
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Partially covering absorber: partcov*xstar500 | ||||||||
NH/1022 |
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log ξ |
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Cf (%) |
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Highly ionized absorber: xstar5000 | ||||||||
NH/1022 |
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log ξ | ![]() |
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υout/c |
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Gaussian emission line: zgauss1 | ||||||||
E (keV) | ≡6.4 | |||||||
σ (eV) |
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I/(10−6) |
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< 3.6 | < 3.2 |
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< 2.2 |
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EW |
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< 200 | < 150 |
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< 140 |
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Gaussian emission line: zgauss2 | ||||||||
E (keV) |
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σ (eV) |
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I/(10−5) |
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EW |
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MOS cross-calibration constant | ||||||||
C |
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Fit statistics | χ2/ν = 2176/1888 | |||||||
Pnull = 4 × 10−6 | ||||||||
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Notes. Units: power-law normalization N1 keV [10−4 photons keV−1 cm−2 s−1]; column density NH [1022 cm−2]; ionization parameter ξ [erg cm s−1]; outflowing velocity υout [c]; Gaussian emission line centroid energy E [keV], width σ [eV], intensity I [10−5 photons cm−2 s−1], equivalent width (EW) [eV]; flux f [10−12 erg s−1 cm−2]; luminosity L [1043 erg s−1]. The parameters kept tied between different epochs are the highly ionized absorber ionization parameter and the Gaussian emission line widths and centroid energies. The unabsorbed flux is corrected for both intrinsic and Galactic absorptions, as is the luminosity.
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