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Table 2.

Summary of best-fit solutions of XMM-Newton and NuSTAR data using different models for MCG-02-12-017.

Model MyTorus MyTorus borus02
Edge-on Face-on
χ2/d.o.f. 192/200 192/200 186/198
CIns1(a) 0.88 0.89 0.89
CIns2(b) 1.24 1.28 1.25
Γ 1.94 1.98 2.11
CTor(c) – – 1.00
θInc(d) – – 49
NH, z(e) 0.26 0.26 0.27
NH, S(f) 2.00 10.0 1.98
fs(g) 10−2 0.25 0.17 0.20
kT (h) 0.46 0.48 0.47
F (i)2 − 10 keV 5.65 5.59 5.55
F (j)10 − 40 keV 1.57 1.65 1.63
L (k)2 − 10 keV 4.98 4.82 5.17
L (l)10 − 40 keV 4.69 4.27 3.77

Notes. We summarise here the best-fits of joint XMM-Newton–NuSTAR spectra using different torus models at 0.6–50 keV. The statistics and degrees of freedom for each fit are also reported.

(a)

CIns1 = CFPMA/PN is the cross calibration constant between NuSTAR observation of 2014 and XMM-Newton observation of 2016.

(b)

CIns2 = CFPMA/PN is the cross calibration constant between NuSTAR observation of 2016 and XMM-Newton observation of 2016.

(c)

Covering factor: fraction of sky covered by the torus, as seen by the nucleus, given by CTor = cos(θTor).

(d)

Inclination angle: angle (in degrees) between the symmetry axis of the torus and the LOS angle.

(e)

“Line of sight” column density in 1024 cm−2.

(f)

Average column density from scattering in 1024 cm−2.

(g)

Fraction of primary emission getting scattered, rather than absorbed by the obscuring material.

(h)

Temperature in the thermal component mekal in keV.

(i)

Flux between 2 and 10 keV in 10−13 erg cm−2 s−1.

(j)

Flux between 10 and 40 keV in 10−12 erg cm−2 s−1.

(k)

Intrinsic luminosity between 2 and 10 keV in 1042 erg s−1.

(l)

Intrinsic luminosity between 10 and 40 keV in 1042 erg s−1.

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