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Table 3

Best fit parameters obtained by fitting the e12 spectrum with different models.

SPECTRUM e12
Shift Shift Shift
LHB-CGM-Coro2-CXBh LHB-CGM-Coro2-CXBs LHB-CGM-Coro2-CXB-PL
SWCX SWCX SWCX
NLHB 2.7 ± 0.5 3.1 ± 0.5 2.7(†) 2.7(†) 2.7(†) 2.7(†)
NCXB 0.343 ± 0.004 0.341 ± 0.004 0.327 ± 0.004 0.325 ± 0.004 0.264 ± 0.005 0.267 ± 0.004
ΓCXBPL 4.3 ± 0.3 4.8 ± 0.4
NCXBPL 0.020 ± 0.006 0.009 ± 0.004
kTCGM 0.157 ± 0.004 0.171 ± 0.006 0.153 ± 0.004 0.167 ± 0.007 0.156 ± 0.003 0.172 ± 0.004
ZCGM 0.057 ± 0.003 0.046 ± 0.003 0.093 ± 0.008 0.089 ± 0.009 0.3(†) 0.3(†)
0.57 ± 0.03
NCGM 65 ± 5 44 ± 4 40 ± 2 22 ± 2 12.5 ± 0.5 7.1 ± 0.4
kTCoro 0.47 ± 0.08 0.45 ± 0.08 0.49 ± 0.11 0.50 ± 0.10 0.49 ± 0.09 0.47 ± 0.09
τ
NCoro 1.0 ± 0.2 1.1 ± 0.2 0.8 ± 0.2 0.8 ± 0.2
χ2 913.1 948.8 923.7 964.3 908.3 933.8
d.o.f. 807 807 808 808 807 807

Notes. The nomenclature is the same as for Table 2. CXBh and CXBs mean that the CXB component has been substituted with the CXBh and CXBs components. CXB-PL considers the CXB component, with the addition of an absorbed power law at low energy (see Sect. 8.2.2). ΓCXBPL and NCXBPL report the photon index and normalization (in units of photons keV−1 cm−2 s−1 at 1 keV) of an additional non-thermal diffuse component.(†) Value fixed in the fit.

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