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Table 2

Hard (4–79 keV) X-ray continuum emission (XMM-Newton +NuSTAR observations): Power law plus reflection models.

Phenomenological reflection model (cut-off-PL + Fe K α emission line + pexrav)
Obs. Obs. NH Γ Ec Energy1 EW 2 Int.3 R (Ω/2π) A norm χ2/ν
N. name (×1022 cm-2) (keV) (keV) (eV) (×10-5) (×10-3)
7 M4N 4.1 ± 0.5 1.74 ± 0.04 >313 6.35 ± 0.02 69 ± 9 3.0 0.56 5.9 3535/3471
11 M8N 1.75 ± 0.06 >212 6.38 ± 0.02 83 ± 10 3.0 0.65 6.2 3535/3471
16 M13N 5.8 1.60 ± 0.04 129 6.42 ± 0.02 110 ± 10 3.7 0.91 5.9 3535/3471
Physical and self-consistent reflection model (cut-off-PL + pexmon)
Obs. Obs. NH Γ Ec R (Ω/2π) A norm χ2/ν
N. name (×1022 cm-2) (keV) (×10-3)
7 M4N 3.8 ± 0.7 1.73 ± 0.02 >310 0.51 5.4 ± 0.5 1234/1157
11 M8N 5.5 ± 0.8 1.63 ± 0.05 157 0.79 6.0 ± 0.5 1178/1157
16 M13N 5.7 ± 1.2 1.60 ± 0.06 123 0.95 6.2 ± 0.5 1153/1157

Notes.

(1)

Emission line rest-frame energy centroid, in units of keV.

(2)

Emission line rest-frame equivalent width in units of eV. The width of the line was fixed to σ = 0.1 keV (see text for details).

(3)

2–10 keV flux in units of 10-11 erg s-1 cm-2.

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