Table 2: Spectral fit results with a PHABS*MEKAL model (see Sect. 4.2). Uncertainties are at the 90% confidence level.
$N_{\rm H}$ kT Z redshift fX [0.5-2.0 keV]$^\ddagger$ fX [2.0-10.0 keV]$^\ddagger$ LX [bolom.]$^\ddagger$ $\chi^{2}_{\nu}/$d.o.f.
(1021 cm-2) (keV) ($Z_{\odot}$)   (10-13 erg cm-2 s-1) (10-13 erg cm-2 s-1) (1044 erg s-1)  
$\rm 1.6^{+0.2}_{-0.1}$ $\rm 4.84^{+0.50}_{-0.42}$ $\rm0.40^{+0.13}_{-0.12}$ $\rm0.263^{+0.012}_{-0.010}$ 4.6 5.8 3.0 1.09/246
$1.39^{\dagger}$ $\rm 5.43^{+0.39}_{-0.38}$ $\rm0.41^{+0.14}_{-0.13}$ $\rm0.264^{+0.015}_{-0.010}$ 4.3 6.0 3.0 1.12/247
$\rm 1.6^{+0.2}_{-0.1}$ $\rm 4.92^{+0.50}_{-0.48}$ $\rm0.38^{+0.12}_{-0.12}$ $0.271^{\ast}$ 4.6 5.8 3.2 1.09/247
$1.39^{\dagger}$ $\rm 5.48^{+0.40}_{-0.39}$ $\rm0.39^{+0.13}_{-0.12}$ $0.271^{\ast}$ 4.3 6.0 3.2 1.12/248
$^\ddagger$ Corrected for absorptions;
$^\dagger$ fixed at the Galactic value (Dickey & Lockman 1990);
$^\ast$ fixed at the optical redshift (Sect. 6).

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