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Table 2:

Best fit parameters of a mekal plus an absorbed power-law model for the Chandra data and an absorbed power-law model for the XMM-Newton spectra.

Obs. ID
Nha $\Gamma $ Pl norm. kTa EMab Fluxc Corr. fluxc Pld
  1020 cm-2   10-4 Photons keV-1 cm-2 s-1 keV 1062 cm-3 10-13 erg s-1 10-13 erg s-1 %
4741 <6.78 2.13 [2.00-2.28] 4.28 [3.92-4.71] 0.62 [0.58-0.66] 2.64 [2.27-2.99] 18.1 [17.1-18.8] 18.5 [18.2-20.1] 94
7077   2.26 [2.16-2.39] 1.82 [1.68-1.99]     7.8 [7.5-7.9] 8.21 [8.0-9.0] 83
7078   2.34 [2.22-2.47] 4.21 [3.90-4.61]     16.0 [14.9-16.2] 16.5 [16.1-18.5] 93
7079   2.38 [2.28-2.50] 3.76 [3.54-4.07]     14.1 [13.3-14.3] 15.05 [14.7-16.4] 90
7080   2.02 [1.84-2.20] 1.10 [0.96-1.26]     5.9 [5.5-6.1] 6.0 [5.7-6.8] 80
7081   2.12 [2.00-2.25] 1.25 [1.14-1.29]     6.2 [5.9-6.4] 6.4 [6.2-7.1] 81
Reduced $\chi^{2} = 0.93$ for 310 d.o.f.
0205010101 3.82 [3.05-4.59] 2.05 [2.03-2.07] 8.07 [7.90-8.24]     33.8 [32.8-33.2] 34.5 [34.2-34.8] 100
Reduced $\chi^{2} = 1.01$ for 487 d.o.f.

Notes. (a) Parameter linked for the different Chandra observations; (b) the emission measure (EM) of the mekal model, $EM=\int$$n_{\rm e}$$n_{\rm H}$dV; (c) fluxes in the 0.5-8 keV energy range; (d) the power-law component fraction to the total corrected flux.


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