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Table 2:

Parameters of the emission lines of the Fe K$\alpha $ complex from a bremsstrahlung + 3 Gaussian lines model.
  $\lambda_{\rm C}$ EW Fluxa
  (Å) (mÅ) ($\times$ 10-5)
all observation:      
Fe K (fluorescence) 1.9312[60] 10[2] $\rm 4.4^{+0.8}_{-1.0}$
Fe XXV 1.8533[55] 12[3] $\rm 5.3^{+1.4}_{-0.9}$
Fe XXVI Ly$\alpha $ 1.7737[51] 7[2] $\rm 3.1^{+0.7}_{-0.5}$
low state:      
Fe K (fluorescence) 1.937[12] 13[5] $\rm 4.1^{+1.0}_{-1.7}$
Fe XXV 1.867[17] 12[4] $\rm 4.1^{+1.5}_{-1.2}$
Fe XXVI Ly$\alpha $ 1.781[10] 7[3] $\rm 2.2^{+0.9}_{-0.8}$
high state:      
Fe K (fluorescence) 1.9282[60] 10[3] $\rm 5.6^{+1.0}_{-1.6}$
Fe XXV 1.8478[83] 13[4] $\rm 7.6^{+2.2}_{-1.4}$
Fe XXVI Ly$\alpha $ 1.7737[76] 8[2] $\rm 4.4^{+1.3}_{-0.9}$

Notes. Quoted errors are at 90% confidence level. The temperature of the bremsstrahlung model at 1.2-4.1 Å (3-10 keV) converges to kT = 13.36(+0.21/-0.25) keV.
(a) Total flux in line, in units of photons cm-2 s-1.


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