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Table A.5.

Summary of best-fit solutions of XMM-Newton, Chandra, and NuSTAR data using different models for 2MASX J20145928+2523010

Model MyTorus MyTorus borus02
Edge-on Face-on
χ2/dof 545/581 545/581 564/580
CIns1a 1.98 1.98 1.98
CIns2b 1.32 1.32 1.31
CIns3c 1.95 1.95 1.94
Γ 1.79 1.77 1.52
CTor — — 1.00
θInc — — 18
NH,zd 2.02 2.04 2.18
NH,Se 11.93 20.15 17.63
fs 10−2 0.68 0.42 1.06
Ff2 − 10keV 1.83 1.83 1.81
F10 − 50keV 5.04 5.07 6.81
L2 − 10keV 6.27 5.95 8.20
L10 − 50keV 8.76 8.52 17.57

Notes. We summarise here the best-fits of joint XMM-Newton, Chandra and NuSTAR spectra using different torus models at 0.6-50 keV, referred to in Section 4.6. 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 = CACIS/PN is the cross-calibration constant between Chandra observation of 2018 and XMM-Newton observation of 2017.

b

CIns2 = CFPMA/PN is the cross-calibration constant between NuSTAR observation of 2017 and XMM-Newton observation of 2017.

c

CIns3 = CFPMA/PN is the cross-calibration constant between NuSTAR observation of 2020 and XMM-Newton observation of 2017.

d

‘Line of sight’ column density in 1022 cm−2.

e

Average column density from scattering in 1022 cm−2.

f

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

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