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Table A.6.

Summary of best-fit solutions of XMM-Newton and NuSTAR data using different models for ESO138-G001

Model MyTorus MyTorus borus02
Edge-on Face-on
χ2/dof 2636/1818 2566/1818 2419/1816
CIns1a 1.15 1.15 1.16
CIns2b 1.07 1.08 1.09
Γ 1.53 1.66 1.98
CTor — — 0.80
θInc — — 18
NH,z 0.33 0.34 0.47
NH,S 1.47 3.00 10.35
Fe Kαc 6.42 6.42 6.44
Fe Kα normd10−5 2.28 1.91 1.04
fs 10−2 7.46 8.14 3.22
kT 0.68 0.68 0.74
Fe2 − 10keV 2.25 2.24 2.24
Ff10 − 50keV 1.42 1.44 1.43
L2 − 10keVg 11.59 12.11 3.61
L10 − 50keVh 24.51 20.90 3.34

Notes. We summarise here the best-fits of joint XMM-Newton–NuSTAR spectra using different torus models at 0.6-50 keV, referred to in Section 4.7. The statistics and degrees of freedom for each fit are also reported. The parameters are reported as in Table 2 if not mentioned otherwise.

a

CIns1 = CFPMA/PN is the cross-calibration constant between NuSTAR observation of 2016 and XMM-Newton observation of 2013.

b

CIns2 = CFPMA/PN is the cross-calibration constant between NuSTAR observation of 2020 and XMM-Newton observation of 2013.

c

Energy of the Iron Kα line in keV.

d

Normalization of line component depicting total photons in cm−2 s−1.

e

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

f

Flux between 10 and 50 keV in 10−11 erg cm−2 s−1.

g

Intrinsic luminosity between 2 and 10 keV in 1041 erg s−1.

h

Intrinsic luminosity between 2 and 10 keV in 1041 erg s−1.

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