Table 2.
Spectral fit results for the baseline model [(partcov*xstar500)*pow].
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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MOS cross-calibration constant | ||||||||
C |
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Fit statistics | χ2/ν = 2779/1923 | |||||||
Pnull = 2 × 10−34 | ||||||||
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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]; flux f [10−12 erg s−1 cm−2]; luminosity L [1043 erg s−1]. The unabsorbed flux is corrected for both intrinsic and Galactic absorption, as is the luminosity.
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